From 198eea453664a5d929bc3c5610584c32116ff517 Mon Sep 17 00:00:00 2001 From: fjosw Date: Tue, 25 Apr 2023 07:26:54 +0000 Subject: [PATCH] Documentation updated --- docs/pyerrors.html | 2 +- docs/pyerrors/correlators.html | 2 +- docs/pyerrors/covobs.html | 2 +- docs/pyerrors/dirac.html | 2 +- docs/pyerrors/fits.html | 2 +- docs/pyerrors/input.html | 2 +- docs/pyerrors/input/bdio.html | 2 +- docs/pyerrors/input/dobs.html | 2 +- docs/pyerrors/input/hadrons.html | 1838 +++++++------- docs/pyerrors/input/json.html | 2 +- docs/pyerrors/input/misc.html | 589 +++-- docs/pyerrors/input/openQCD.html | 3838 +++++++++++++++--------------- docs/pyerrors/input/pandas.html | 2 +- docs/pyerrors/input/sfcf.html | 2 +- docs/pyerrors/input/utils.html | 2 +- docs/pyerrors/linalg.html | 2 +- docs/pyerrors/misc.html | 2 +- docs/pyerrors/mpm.html | 2 +- docs/pyerrors/obs.html | 2 +- docs/pyerrors/roots.html | 2 +- docs/pyerrors/version.html | 2 +- docs/search.js | 2 +- 22 files changed, 3243 insertions(+), 3060 deletions(-) diff --git a/docs/pyerrors.html b/docs/pyerrors.html index a520da02..1f1f3ca0 100644 --- a/docs/pyerrors.html +++ b/docs/pyerrors.html @@ -3,7 +3,7 @@ - + pyerrors API documentation diff --git a/docs/pyerrors/correlators.html b/docs/pyerrors/correlators.html index d78bbcf1..f1deecac 100644 --- a/docs/pyerrors/correlators.html +++ b/docs/pyerrors/correlators.html @@ -3,7 +3,7 @@ - + pyerrors.correlators API documentation diff --git a/docs/pyerrors/covobs.html b/docs/pyerrors/covobs.html index afab0f72..8c1ba353 100644 --- a/docs/pyerrors/covobs.html +++ b/docs/pyerrors/covobs.html @@ -3,7 +3,7 @@ - + pyerrors.covobs API documentation diff --git a/docs/pyerrors/dirac.html b/docs/pyerrors/dirac.html index 8ec4e924..62fabbd2 100644 --- a/docs/pyerrors/dirac.html +++ b/docs/pyerrors/dirac.html @@ -3,7 +3,7 @@ - + pyerrors.dirac API documentation diff --git a/docs/pyerrors/fits.html b/docs/pyerrors/fits.html index a37db5bb..96b55029 100644 --- a/docs/pyerrors/fits.html +++ b/docs/pyerrors/fits.html @@ -3,7 +3,7 @@ - + pyerrors.fits API documentation diff --git a/docs/pyerrors/input.html b/docs/pyerrors/input.html index 9e8e68fe..59675da6 100644 --- a/docs/pyerrors/input.html +++ b/docs/pyerrors/input.html @@ -3,7 +3,7 @@ - + pyerrors.input API documentation diff --git a/docs/pyerrors/input/bdio.html b/docs/pyerrors/input/bdio.html index 0e74f042..6924fbb5 100644 --- a/docs/pyerrors/input/bdio.html +++ b/docs/pyerrors/input/bdio.html @@ -3,7 +3,7 @@ - + pyerrors.input.bdio API documentation diff --git a/docs/pyerrors/input/dobs.html b/docs/pyerrors/input/dobs.html index c4eb0f2f..d85a2e46 100644 --- a/docs/pyerrors/input/dobs.html +++ b/docs/pyerrors/input/dobs.html @@ -3,7 +3,7 @@ - + pyerrors.input.dobs API documentation diff --git a/docs/pyerrors/input/hadrons.html b/docs/pyerrors/input/hadrons.html index 97339c92..3c974861 100644 --- a/docs/pyerrors/input/hadrons.html +++ b/docs/pyerrors/input/hadrons.html @@ -3,7 +3,7 @@ - + pyerrors.input.hadrons API documentation @@ -55,6 +55,9 @@
  • read_meson_hd5
  • +
  • + extract_t0_hd5 +
  • read_DistillationContraction_hd5
  • @@ -105,489 +108,556 @@ 6from ..obs import Obs, CObs 7from ..correlators import Corr 8from ..dirac import epsilon_tensor_rank4 - 9 + 9from .misc import fit_t0 10 - 11def _get_files(path, filestem, idl): - 12 ls = os.listdir(path) - 13 - 14 # Clean up file list - 15 files = list(filter(lambda x: x.startswith(filestem + "."), ls)) - 16 - 17 if not files: - 18 raise Exception('No files starting with', filestem, 'in folder', path) - 19 - 20 def get_cnfg_number(n): - 21 return int(n.replace(".h5", "")[len(filestem) + 1:]) # From python 3.9 onward the safer 'removesuffix' method can be used. - 22 - 23 # Sort according to configuration number - 24 files.sort(key=get_cnfg_number) - 25 - 26 cnfg_numbers = [] - 27 filtered_files = [] - 28 for line in files: - 29 no = get_cnfg_number(line) - 30 if idl: - 31 if no in list(idl): - 32 filtered_files.append(line) - 33 cnfg_numbers.append(no) - 34 else: - 35 filtered_files.append(line) - 36 cnfg_numbers.append(no) - 37 - 38 if idl: - 39 if Counter(list(idl)) != Counter(cnfg_numbers): - 40 raise Exception("Not all configurations specified in idl found, configurations " + str(list(Counter(list(idl)) - Counter(cnfg_numbers))) + " are missing.") - 41 - 42 # Check that configurations are evenly spaced - 43 dc = np.unique(np.diff(cnfg_numbers)) - 44 if np.any(dc < 0): - 45 raise Exception("Unsorted files") - 46 if len(dc) == 1: - 47 idx = range(cnfg_numbers[0], cnfg_numbers[-1] + dc[0], dc[0]) - 48 elif idl: - 49 idx = idl - 50 else: - 51 raise Exception("Configurations are not evenly spaced. Provide an idl if you want to proceed with this set of configurations.") - 52 - 53 return filtered_files, idx - 54 + 11 + 12def _get_files(path, filestem, idl): + 13 ls = os.listdir(path) + 14 + 15 # Clean up file list + 16 files = list(filter(lambda x: x.startswith(filestem + "."), ls)) + 17 + 18 if not files: + 19 raise Exception('No files starting with', filestem, 'in folder', path) + 20 + 21 def get_cnfg_number(n): + 22 return int(n.replace(".h5", "")[len(filestem) + 1:]) # From python 3.9 onward the safer 'removesuffix' method can be used. + 23 + 24 # Sort according to configuration number + 25 files.sort(key=get_cnfg_number) + 26 + 27 cnfg_numbers = [] + 28 filtered_files = [] + 29 for line in files: + 30 no = get_cnfg_number(line) + 31 if idl: + 32 if no in list(idl): + 33 filtered_files.append(line) + 34 cnfg_numbers.append(no) + 35 else: + 36 filtered_files.append(line) + 37 cnfg_numbers.append(no) + 38 + 39 if idl: + 40 if Counter(list(idl)) != Counter(cnfg_numbers): + 41 raise Exception("Not all configurations specified in idl found, configurations " + str(list(Counter(list(idl)) - Counter(cnfg_numbers))) + " are missing.") + 42 + 43 # Check that configurations are evenly spaced + 44 dc = np.unique(np.diff(cnfg_numbers)) + 45 if np.any(dc < 0): + 46 raise Exception("Unsorted files") + 47 if len(dc) == 1: + 48 idx = range(cnfg_numbers[0], cnfg_numbers[-1] + dc[0], dc[0]) + 49 elif idl: + 50 idx = idl + 51 else: + 52 raise Exception("Configurations are not evenly spaced. Provide an idl if you want to proceed with this set of configurations.") + 53 + 54 return filtered_files, idx 55 - 56def read_meson_hd5(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None): - 57 r'''Read hadrons meson hdf5 file and extract the meson labeled 'meson' - 58 - 59 Parameters - 60 ----------------- - 61 path : str - 62 path to the files to read - 63 filestem : str - 64 namestem of the files to read - 65 ens_id : str - 66 name of the ensemble, required for internal bookkeeping - 67 meson : str - 68 label of the meson to be extracted, standard value meson_0 which - 69 corresponds to the pseudoscalar pseudoscalar two-point function. - 70 gammas : tuple of strings - 71 Instrad of a meson label one can also provide a tuple of two strings - 72 indicating the gamma matrices at source and sink. - 73 ("Gamma5", "Gamma5") corresponds to the pseudoscalar pseudoscalar - 74 two-point function. The gammas argument dominateds over meson. - 75 idl : range - 76 If specified only configurations in the given range are read in. - 77 - 78 Returns - 79 ------- - 80 corr : Corr - 81 Correlator of the source sink combination in question. - 82 ''' - 83 - 84 files, idx = _get_files(path, filestem, idl) - 85 - 86 tree = meson.rsplit('_')[0] - 87 if gammas is not None: - 88 h5file = h5py.File(path + '/' + files[0], "r") - 89 found_meson = None - 90 for key in h5file[tree].keys(): - 91 if gammas[0] == h5file[tree][key].attrs["gamma_snk"][0].decode() and h5file[tree][key].attrs["gamma_src"][0].decode() == gammas[1]: - 92 found_meson = key - 93 break - 94 h5file.close() - 95 if found_meson: - 96 meson = found_meson - 97 else: - 98 raise Exception("Source Sink combination " + str(gammas) + " not found.") - 99 -100 corr_data = [] -101 infos = [] -102 for hd5_file in files: -103 h5file = h5py.File(path + '/' + hd5_file, "r") -104 if not tree + '/' + meson in h5file: -105 raise Exception("Entry '" + meson + "' not contained in the files.") -106 raw_data = h5file[tree + '/' + meson + '/corr'] -107 real_data = raw_data[:]["re"].astype(np.double) -108 corr_data.append(real_data) -109 if not infos: -110 for k, i in h5file[tree + '/' + meson].attrs.items(): -111 infos.append(k + ': ' + i[0].decode()) -112 h5file.close() -113 corr_data = np.array(corr_data) -114 -115 l_obs = [] -116 for c in corr_data.T: -117 l_obs.append(Obs([c], [ens_id], idl=[idx])) -118 -119 corr = Corr(l_obs) -120 corr.tag = r", ".join(infos) -121 return corr -122 + 56 + 57def read_meson_hd5(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None): + 58 r'''Read hadrons meson hdf5 file and extract the meson labeled 'meson' + 59 + 60 Parameters + 61 ----------------- + 62 path : str + 63 path to the files to read + 64 filestem : str + 65 namestem of the files to read + 66 ens_id : str + 67 name of the ensemble, required for internal bookkeeping + 68 meson : str + 69 label of the meson to be extracted, standard value meson_0 which + 70 corresponds to the pseudoscalar pseudoscalar two-point function. + 71 gammas : tuple of strings + 72 Instrad of a meson label one can also provide a tuple of two strings + 73 indicating the gamma matrices at source and sink. + 74 ("Gamma5", "Gamma5") corresponds to the pseudoscalar pseudoscalar + 75 two-point function. The gammas argument dominateds over meson. + 76 idl : range + 77 If specified only configurations in the given range are read in. + 78 + 79 Returns + 80 ------- + 81 corr : Corr + 82 Correlator of the source sink combination in question. + 83 ''' + 84 + 85 files, idx = _get_files(path, filestem, idl) + 86 + 87 tree = meson.rsplit('_')[0] + 88 if gammas is not None: + 89 h5file = h5py.File(path + '/' + files[0], "r") + 90 found_meson = None + 91 for key in h5file[tree].keys(): + 92 if gammas[0] == h5file[tree][key].attrs["gamma_snk"][0].decode() and h5file[tree][key].attrs["gamma_src"][0].decode() == gammas[1]: + 93 found_meson = key + 94 break + 95 h5file.close() + 96 if found_meson: + 97 meson = found_meson + 98 else: + 99 raise Exception("Source Sink combination " + str(gammas) + " not found.") +100 +101 corr_data = [] +102 infos = [] +103 for hd5_file in files: +104 h5file = h5py.File(path + '/' + hd5_file, "r") +105 if not tree + '/' + meson in h5file: +106 raise Exception("Entry '" + meson + "' not contained in the files.") +107 raw_data = h5file[tree + '/' + meson + '/corr'] +108 real_data = raw_data[:]["re"].astype(np.double) +109 corr_data.append(real_data) +110 if not infos: +111 for k, i in h5file[tree + '/' + meson].attrs.items(): +112 infos.append(k + ': ' + i[0].decode()) +113 h5file.close() +114 corr_data = np.array(corr_data) +115 +116 l_obs = [] +117 for c in corr_data.T: +118 l_obs.append(Obs([c], [ens_id], idl=[idx])) +119 +120 corr = Corr(l_obs) +121 corr.tag = r", ".join(infos) +122 return corr 123 -124def read_DistillationContraction_hd5(path, ens_id, diagrams=["direct"], idl=None): -125 """Read hadrons DistillationContraction hdf5 files in given directory structure -126 -127 Parameters -128 ----------------- -129 path : str -130 path to the directories to read -131 ens_id : str -132 name of the ensemble, required for internal bookkeeping -133 diagrams : list -134 List of strings of the diagrams to extract, e.g. ["direct", "box", "cross"]. -135 idl : range -136 If specified only configurations in the given range are read in. -137 -138 Returns -139 ------- -140 result : dict -141 extracted DistillationContration data -142 """ -143 -144 res_dict = {} +124 +125def _extract_real_arrays(path, files, tree, keys): +126 corr_data = {} +127 for key in keys: +128 corr_data[key] = [] +129 for hd5_file in files: +130 h5file = h5py.File(path + '/' + hd5_file, "r") +131 for key in keys: +132 if not tree + '/' + key in h5file: +133 raise Exception("Entry '" + key + "' not contained in the files.") +134 raw_data = h5file[tree + '/' + key + '/data'] +135 real_data = raw_data[:].astype(np.double) +136 corr_data[key].append(real_data) +137 h5file.close() +138 for key in keys: +139 corr_data[key] = np.array(corr_data[key]) +140 return corr_data +141 +142 +143def extract_t0_hd5(path, filestem, ens_id, obs='Clover energy density', fit_range=5, idl=None, **kwargs): +144 r'''Read hadrons FlowObservables hdf5 file and extract t0 145 -146 directories, idx = _get_files(path, "data", idl) -147 -148 explore_path = Path(path + "/" + directories[0]) -149 -150 for explore_file in explore_path.iterdir(): -151 if explore_file.is_file(): -152 stem = explore_file.with_suffix("").with_suffix("").as_posix().split("/")[-1] -153 else: -154 continue -155 -156 file_list = [] -157 for dir in directories: -158 tmp_path = Path(path + "/" + dir) -159 file_list.append((tmp_path / stem).as_posix() + tmp_path.suffix + ".h5") -160 -161 corr_data = {} -162 -163 for diagram in diagrams: -164 corr_data[diagram] = [] +146 Parameters +147 ----------------- +148 path : str +149 path to the files to read +150 filestem : str +151 namestem of the files to read +152 ens_id : str +153 name of the ensemble, required for internal bookkeeping +154 obs : str +155 label of the observable from which t0 should be extracted. +156 Options: 'Clover energy density' and 'Plaquette energy density' +157 fit_range : int +158 Number of data points left and right of the zero +159 crossing to be included in the linear fit. (Default: 5) +160 idl : range +161 If specified only configurations in the given range are read in. +162 plot_fit : bool +163 If true, the fit for the extraction of t0 is shown together with the data. +164 ''' 165 -166 try: -167 for n_file, (hd5_file, n_traj) in enumerate(zip(file_list, list(idx))): -168 h5file = h5py.File(hd5_file) -169 -170 if n_file == 0: -171 if h5file["DistillationContraction/Metadata"].attrs.get("TimeSources")[0].decode() != "0...": -172 raise Exception("Routine is only implemented for files containing inversions on all timeslices.") -173 -174 Nt = h5file["DistillationContraction/Metadata"].attrs.get("Nt")[0] -175 -176 identifier = [] -177 for in_file in range(len(h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.keys()) - 1): -178 encoded_info = h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.get("DmfInputFiles_" + str(in_file)) -179 full_info = encoded_info[0].decode().split("/")[-1].replace(".h5", "").split("_") -180 my_tuple = (full_info[0], full_info[1][1:], full_info[2], full_info[3]) -181 identifier.append(my_tuple) -182 identifier = tuple(identifier) -183 # "DistillationContraction/Metadata/DmfSuffix" contains info about different quarks, irrelevant in the SU(3) case. -184 -185 for diagram in diagrams: -186 -187 if diagram == "triangle" and "Identity" not in str(identifier): -188 part = "im" -189 else: -190 part = "re" -191 -192 real_data = np.zeros(Nt) -193 for x0 in range(Nt): -194 raw_data = h5file["DistillationContraction/Correlators/" + diagram + "/" + str(x0)][:][part].astype(np.double) -195 real_data += np.roll(raw_data, -x0) -196 real_data /= Nt -197 -198 corr_data[diagram].append(real_data) -199 h5file.close() -200 -201 res_dict[str(identifier)] = {} -202 -203 for diagram in diagrams: +166 files, idx = _get_files(path, filestem, idl) +167 tree = "FlowObservables" +168 +169 h5file = h5py.File(path + '/' + files[0], "r") +170 obs_key = None +171 for key in h5file[tree].keys(): +172 if obs == h5file[tree][key].attrs["description"][0].decode(): +173 obs_key = key +174 break +175 h5file.close() +176 if obs_key is None: +177 raise Exception(f"Observable {obs} not found.") +178 +179 corr_data = _extract_real_arrays(path, files, tree, ["FlowObservables_0", obs_key]) +180 +181 if not np.allclose(corr_data["FlowObservables_0"][0], corr_data["FlowObservables_0"][:]): +182 raise Exception("Not all flow times were equal.") +183 +184 t2E_dict = {} +185 for t2, dat in zip(corr_data["FlowObservables_0"][0], corr_data[obs_key].T): +186 t2E_dict[t2] = Obs([dat], [ens_id], idl=[idx]) - 0.3 +187 +188 return fit_t0(t2E_dict, fit_range, plot_fit=kwargs.get('plot_fit')) +189 +190 +191def read_DistillationContraction_hd5(path, ens_id, diagrams=["direct"], idl=None): +192 """Read hadrons DistillationContraction hdf5 files in given directory structure +193 +194 Parameters +195 ----------------- +196 path : str +197 path to the directories to read +198 ens_id : str +199 name of the ensemble, required for internal bookkeeping +200 diagrams : list +201 List of strings of the diagrams to extract, e.g. ["direct", "box", "cross"]. +202 idl : range +203 If specified only configurations in the given range are read in. 204 -205 tmp_data = np.array(corr_data[diagram]) -206 -207 l_obs = [] -208 for c in tmp_data.T: -209 l_obs.append(Obs([c], [ens_id], idl=[idx])) +205 Returns +206 ------- +207 result : dict +208 extracted DistillationContration data +209 """ 210 -211 corr = Corr(l_obs) -212 corr.tag = str(identifier) -213 -214 res_dict[str(identifier)][diagram] = corr -215 except FileNotFoundError: -216 print("Skip", stem) -217 -218 return res_dict -219 -220 -221class Npr_matrix(np.ndarray): +211 res_dict = {} +212 +213 directories, idx = _get_files(path, "data", idl) +214 +215 explore_path = Path(path + "/" + directories[0]) +216 +217 for explore_file in explore_path.iterdir(): +218 if explore_file.is_file(): +219 stem = explore_file.with_suffix("").with_suffix("").as_posix().split("/")[-1] +220 else: +221 continue 222 -223 def __new__(cls, input_array, mom_in=None, mom_out=None): -224 obj = np.asarray(input_array).view(cls) -225 obj.mom_in = mom_in -226 obj.mom_out = mom_out -227 return obj -228 -229 @property -230 def g5H(self): -231 """Gamma_5 hermitean conjugate +223 file_list = [] +224 for dir in directories: +225 tmp_path = Path(path + "/" + dir) +226 file_list.append((tmp_path / stem).as_posix() + tmp_path.suffix + ".h5") +227 +228 corr_data = {} +229 +230 for diagram in diagrams: +231 corr_data[diagram] = [] 232 -233 Uses the fact that the propagator is gamma5 hermitean, so just the -234 in and out momenta of the propagator are exchanged. -235 """ -236 return Npr_matrix(self, -237 mom_in=self.mom_out, -238 mom_out=self.mom_in) -239 -240 def _propagate_mom(self, other, name): -241 s_mom = getattr(self, name, None) -242 o_mom = getattr(other, name, None) -243 if s_mom is not None and o_mom is not None: -244 if not np.allclose(s_mom, o_mom): -245 raise Exception(name + ' does not match.') -246 return o_mom if o_mom is not None else s_mom -247 -248 def __matmul__(self, other): -249 return self.__new__(Npr_matrix, -250 super().__matmul__(other), -251 self._propagate_mom(other, 'mom_in'), -252 self._propagate_mom(other, 'mom_out')) +233 try: +234 for n_file, (hd5_file, n_traj) in enumerate(zip(file_list, list(idx))): +235 h5file = h5py.File(hd5_file) +236 +237 if n_file == 0: +238 if h5file["DistillationContraction/Metadata"].attrs.get("TimeSources")[0].decode() != "0...": +239 raise Exception("Routine is only implemented for files containing inversions on all timeslices.") +240 +241 Nt = h5file["DistillationContraction/Metadata"].attrs.get("Nt")[0] +242 +243 identifier = [] +244 for in_file in range(len(h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.keys()) - 1): +245 encoded_info = h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.get("DmfInputFiles_" + str(in_file)) +246 full_info = encoded_info[0].decode().split("/")[-1].replace(".h5", "").split("_") +247 my_tuple = (full_info[0], full_info[1][1:], full_info[2], full_info[3]) +248 identifier.append(my_tuple) +249 identifier = tuple(identifier) +250 # "DistillationContraction/Metadata/DmfSuffix" contains info about different quarks, irrelevant in the SU(3) case. +251 +252 for diagram in diagrams: 253 -254 def __array_finalize__(self, obj): -255 if obj is None: -256 return -257 self.mom_in = getattr(obj, 'mom_in', None) -258 self.mom_out = getattr(obj, 'mom_out', None) -259 -260 -261def read_ExternalLeg_hd5(path, filestem, ens_id, idl=None): -262 """Read hadrons ExternalLeg hdf5 file and output an array of CObs -263 -264 Parameters -265 ---------- -266 path : str -267 path to the files to read -268 filestem : str -269 namestem of the files to read -270 ens_id : str -271 name of the ensemble, required for internal bookkeeping -272 idl : range -273 If specified only configurations in the given range are read in. -274 -275 Returns -276 ------- -277 result : Npr_matrix -278 read Cobs-matrix -279 """ +254 if diagram == "triangle" and "Identity" not in str(identifier): +255 part = "im" +256 else: +257 part = "re" +258 +259 real_data = np.zeros(Nt) +260 for x0 in range(Nt): +261 raw_data = h5file["DistillationContraction/Correlators/" + diagram + "/" + str(x0)][:][part].astype(np.double) +262 real_data += np.roll(raw_data, -x0) +263 real_data /= Nt +264 +265 corr_data[diagram].append(real_data) +266 h5file.close() +267 +268 res_dict[str(identifier)] = {} +269 +270 for diagram in diagrams: +271 +272 tmp_data = np.array(corr_data[diagram]) +273 +274 l_obs = [] +275 for c in tmp_data.T: +276 l_obs.append(Obs([c], [ens_id], idl=[idx])) +277 +278 corr = Corr(l_obs) +279 corr.tag = str(identifier) 280 -281 files, idx = _get_files(path, filestem, idl) -282 -283 mom = None +281 res_dict[str(identifier)][diagram] = corr +282 except FileNotFoundError: +283 print("Skip", stem) 284 -285 corr_data = [] -286 for hd5_file in files: -287 file = h5py.File(path + '/' + hd5_file, "r") -288 raw_data = file['ExternalLeg/corr'][0][0].view('complex') -289 corr_data.append(raw_data) -290 if mom is None: -291 mom = np.array(str(file['ExternalLeg/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) -292 file.close() -293 corr_data = np.array(corr_data) -294 -295 rolled_array = np.rollaxis(corr_data, 0, 5) -296 -297 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) -298 for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]): -299 real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx]) -300 imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx]) -301 matrix[si, sj, ci, cj] = CObs(real, imag) -302 -303 return Npr_matrix(matrix, mom_in=mom) -304 -305 -306def read_Bilinear_hd5(path, filestem, ens_id, idl=None): -307 """Read hadrons Bilinear hdf5 file and output an array of CObs -308 -309 Parameters -310 ---------- -311 path : str -312 path to the files to read -313 filestem : str -314 namestem of the files to read -315 ens_id : str -316 name of the ensemble, required for internal bookkeeping -317 idl : range -318 If specified only configurations in the given range are read in. -319 -320 Returns -321 ------- -322 result_dict: dict[Npr_matrix] -323 extracted Bilinears -324 """ -325 -326 files, idx = _get_files(path, filestem, idl) +285 return res_dict +286 +287 +288class Npr_matrix(np.ndarray): +289 +290 def __new__(cls, input_array, mom_in=None, mom_out=None): +291 obj = np.asarray(input_array).view(cls) +292 obj.mom_in = mom_in +293 obj.mom_out = mom_out +294 return obj +295 +296 @property +297 def g5H(self): +298 """Gamma_5 hermitean conjugate +299 +300 Uses the fact that the propagator is gamma5 hermitean, so just the +301 in and out momenta of the propagator are exchanged. +302 """ +303 return Npr_matrix(self, +304 mom_in=self.mom_out, +305 mom_out=self.mom_in) +306 +307 def _propagate_mom(self, other, name): +308 s_mom = getattr(self, name, None) +309 o_mom = getattr(other, name, None) +310 if s_mom is not None and o_mom is not None: +311 if not np.allclose(s_mom, o_mom): +312 raise Exception(name + ' does not match.') +313 return o_mom if o_mom is not None else s_mom +314 +315 def __matmul__(self, other): +316 return self.__new__(Npr_matrix, +317 super().__matmul__(other), +318 self._propagate_mom(other, 'mom_in'), +319 self._propagate_mom(other, 'mom_out')) +320 +321 def __array_finalize__(self, obj): +322 if obj is None: +323 return +324 self.mom_in = getattr(obj, 'mom_in', None) +325 self.mom_out = getattr(obj, 'mom_out', None) +326 327 -328 mom_in = None -329 mom_out = None +328def read_ExternalLeg_hd5(path, filestem, ens_id, idl=None): +329 """Read hadrons ExternalLeg hdf5 file and output an array of CObs 330 -331 corr_data = {} -332 for hd5_file in files: -333 file = h5py.File(path + '/' + hd5_file, "r") -334 for i in range(16): -335 name = file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['gamma'][0].decode('UTF-8') -336 if name not in corr_data: -337 corr_data[name] = [] -338 raw_data = file['Bilinear/Bilinear_' + str(i) + '/corr'][0][0].view('complex') -339 corr_data[name].append(raw_data) -340 if mom_in is None: -341 mom_in = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) -342 if mom_out is None: -343 mom_out = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float) -344 -345 file.close() -346 -347 result_dict = {} -348 -349 for key, data in corr_data.items(): -350 local_data = np.array(data) +331 Parameters +332 ---------- +333 path : str +334 path to the files to read +335 filestem : str +336 namestem of the files to read +337 ens_id : str +338 name of the ensemble, required for internal bookkeeping +339 idl : range +340 If specified only configurations in the given range are read in. +341 +342 Returns +343 ------- +344 result : Npr_matrix +345 read Cobs-matrix +346 """ +347 +348 files, idx = _get_files(path, filestem, idl) +349 +350 mom = None 351 -352 rolled_array = np.rollaxis(local_data, 0, 5) -353 -354 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) -355 for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]): -356 real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx]) -357 imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx]) -358 matrix[si, sj, ci, cj] = CObs(real, imag) -359 -360 result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out) +352 corr_data = [] +353 for hd5_file in files: +354 file = h5py.File(path + '/' + hd5_file, "r") +355 raw_data = file['ExternalLeg/corr'][0][0].view('complex') +356 corr_data.append(raw_data) +357 if mom is None: +358 mom = np.array(str(file['ExternalLeg/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) +359 file.close() +360 corr_data = np.array(corr_data) 361 -362 return result_dict +362 rolled_array = np.rollaxis(corr_data, 0, 5) 363 -364 -365def read_Fourquark_hd5(path, filestem, ens_id, idl=None, vertices=["VA", "AV"]): -366 """Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs -367 -368 Parameters -369 ---------- -370 path : str -371 path to the files to read -372 filestem : str -373 namestem of the files to read -374 ens_id : str -375 name of the ensemble, required for internal bookkeeping -376 idl : range -377 If specified only configurations in the given range are read in. -378 vertices : list -379 Vertex functions to be extracted. -380 -381 Returns -382 ------- -383 result_dict : dict -384 extracted fourquark matrizes -385 """ +364 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) +365 for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]): +366 real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx]) +367 imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx]) +368 matrix[si, sj, ci, cj] = CObs(real, imag) +369 +370 return Npr_matrix(matrix, mom_in=mom) +371 +372 +373def read_Bilinear_hd5(path, filestem, ens_id, idl=None): +374 """Read hadrons Bilinear hdf5 file and output an array of CObs +375 +376 Parameters +377 ---------- +378 path : str +379 path to the files to read +380 filestem : str +381 namestem of the files to read +382 ens_id : str +383 name of the ensemble, required for internal bookkeeping +384 idl : range +385 If specified only configurations in the given range are read in. 386 -387 files, idx = _get_files(path, filestem, idl) -388 -389 mom_in = None -390 mom_out = None -391 -392 vertex_names = [] -393 for vertex in vertices: -394 vertex_names += _get_lorentz_names(vertex) -395 -396 corr_data = {} +387 Returns +388 ------- +389 result_dict: dict[Npr_matrix] +390 extracted Bilinears +391 """ +392 +393 files, idx = _get_files(path, filestem, idl) +394 +395 mom_in = None +396 mom_out = None 397 -398 tree = 'FourQuarkFullyConnected/FourQuarkFullyConnected_' -399 -400 for hd5_file in files: -401 file = h5py.File(path + '/' + hd5_file, "r") -402 -403 for i in range(32): -404 name = (file[tree + str(i) + '/info'].attrs['gammaA'][0].decode('UTF-8'), file[tree + str(i) + '/info'].attrs['gammaB'][0].decode('UTF-8')) -405 if name in vertex_names: -406 if name not in corr_data: -407 corr_data[name] = [] -408 raw_data = file[tree + str(i) + '/corr'][0][0].view('complex') -409 corr_data[name].append(raw_data) -410 if mom_in is None: -411 mom_in = np.array(str(file[tree + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) -412 if mom_out is None: -413 mom_out = np.array(str(file[tree + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float) -414 -415 file.close() -416 -417 intermediate_dict = {} +398 corr_data = {} +399 for hd5_file in files: +400 file = h5py.File(path + '/' + hd5_file, "r") +401 for i in range(16): +402 name = file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['gamma'][0].decode('UTF-8') +403 if name not in corr_data: +404 corr_data[name] = [] +405 raw_data = file['Bilinear/Bilinear_' + str(i) + '/corr'][0][0].view('complex') +406 corr_data[name].append(raw_data) +407 if mom_in is None: +408 mom_in = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) +409 if mom_out is None: +410 mom_out = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float) +411 +412 file.close() +413 +414 result_dict = {} +415 +416 for key, data in corr_data.items(): +417 local_data = np.array(data) 418 -419 for vertex in vertices: -420 lorentz_names = _get_lorentz_names(vertex) -421 for v_name in lorentz_names: -422 if v_name in [('SigmaXY', 'SigmaZT'), -423 ('SigmaXT', 'SigmaYZ'), -424 ('SigmaYZ', 'SigmaXT'), -425 ('SigmaZT', 'SigmaXY')]: -426 sign = -1 -427 else: -428 sign = 1 -429 if vertex not in intermediate_dict: -430 intermediate_dict[vertex] = sign * np.array(corr_data[v_name]) -431 else: -432 intermediate_dict[vertex] += sign * np.array(corr_data[v_name]) -433 -434 result_dict = {} -435 -436 for key, data in intermediate_dict.items(): -437 -438 rolled_array = np.moveaxis(data, 0, 8) -439 -440 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) -441 for index in np.ndindex(rolled_array.shape[:-1]): -442 real = Obs([rolled_array[index].real], [ens_id], idl=[idx]) -443 imag = Obs([rolled_array[index].imag], [ens_id], idl=[idx]) -444 matrix[index] = CObs(real, imag) -445 -446 result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out) +419 rolled_array = np.rollaxis(local_data, 0, 5) +420 +421 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) +422 for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]): +423 real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx]) +424 imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx]) +425 matrix[si, sj, ci, cj] = CObs(real, imag) +426 +427 result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out) +428 +429 return result_dict +430 +431 +432def read_Fourquark_hd5(path, filestem, ens_id, idl=None, vertices=["VA", "AV"]): +433 """Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs +434 +435 Parameters +436 ---------- +437 path : str +438 path to the files to read +439 filestem : str +440 namestem of the files to read +441 ens_id : str +442 name of the ensemble, required for internal bookkeeping +443 idl : range +444 If specified only configurations in the given range are read in. +445 vertices : list +446 Vertex functions to be extracted. 447 -448 return result_dict -449 -450 -451def _get_lorentz_names(name): -452 lorentz_index = ['X', 'Y', 'Z', 'T'] +448 Returns +449 ------- +450 result_dict : dict +451 extracted fourquark matrizes +452 """ 453 -454 res = [] +454 files, idx = _get_files(path, filestem, idl) 455 -456 if name == "TT": -457 for i in range(4): -458 for j in range(i + 1, 4): -459 res.append(("Sigma" + lorentz_index[i] + lorentz_index[j], "Sigma" + lorentz_index[i] + lorentz_index[j])) -460 return res -461 -462 if name == "TTtilde": -463 for i in range(4): -464 for j in range(i + 1, 4): -465 for k in range(4): -466 for o in range(k + 1, 4): -467 fac = epsilon_tensor_rank4(i, j, k, o) -468 if not np.isclose(fac, 0.0): -469 res.append(("Sigma" + lorentz_index[i] + lorentz_index[j], "Sigma" + lorentz_index[k] + lorentz_index[o])) -470 return res -471 -472 assert len(name) == 2 -473 -474 if 'S' in name or 'P' in name: -475 if not set(name) <= set(['S', 'P']): -476 raise Exception("'" + name + "' is not a Lorentz scalar") -477 -478 g_names = {'S': 'Identity', -479 'P': 'Gamma5'} -480 -481 res.append((g_names[name[0]], g_names[name[1]])) -482 -483 else: -484 if not set(name) <= set(['V', 'A']): -485 raise Exception("'" + name + "' is not a Lorentz scalar") -486 -487 for ind in lorentz_index: -488 res.append(('Gamma' + ind + (name[0] == 'A') * 'Gamma5', -489 'Gamma' + ind + (name[1] == 'A') * 'Gamma5')) -490 -491 return res +456 mom_in = None +457 mom_out = None +458 +459 vertex_names = [] +460 for vertex in vertices: +461 vertex_names += _get_lorentz_names(vertex) +462 +463 corr_data = {} +464 +465 tree = 'FourQuarkFullyConnected/FourQuarkFullyConnected_' +466 +467 for hd5_file in files: +468 file = h5py.File(path + '/' + hd5_file, "r") +469 +470 for i in range(32): +471 name = (file[tree + str(i) + '/info'].attrs['gammaA'][0].decode('UTF-8'), file[tree + str(i) + '/info'].attrs['gammaB'][0].decode('UTF-8')) +472 if name in vertex_names: +473 if name not in corr_data: +474 corr_data[name] = [] +475 raw_data = file[tree + str(i) + '/corr'][0][0].view('complex') +476 corr_data[name].append(raw_data) +477 if mom_in is None: +478 mom_in = np.array(str(file[tree + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float) +479 if mom_out is None: +480 mom_out = np.array(str(file[tree + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float) +481 +482 file.close() +483 +484 intermediate_dict = {} +485 +486 for vertex in vertices: +487 lorentz_names = _get_lorentz_names(vertex) +488 for v_name in lorentz_names: +489 if v_name in [('SigmaXY', 'SigmaZT'), +490 ('SigmaXT', 'SigmaYZ'), +491 ('SigmaYZ', 'SigmaXT'), +492 ('SigmaZT', 'SigmaXY')]: +493 sign = -1 +494 else: +495 sign = 1 +496 if vertex not in intermediate_dict: +497 intermediate_dict[vertex] = sign * np.array(corr_data[v_name]) +498 else: +499 intermediate_dict[vertex] += sign * np.array(corr_data[v_name]) +500 +501 result_dict = {} +502 +503 for key, data in intermediate_dict.items(): +504 +505 rolled_array = np.moveaxis(data, 0, 8) +506 +507 matrix = np.empty((rolled_array.shape[:-1]), dtype=object) +508 for index in np.ndindex(rolled_array.shape[:-1]): +509 real = Obs([rolled_array[index].real], [ens_id], idl=[idx]) +510 imag = Obs([rolled_array[index].imag], [ens_id], idl=[idx]) +511 matrix[index] = CObs(real, imag) +512 +513 result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out) +514 +515 return result_dict +516 +517 +518def _get_lorentz_names(name): +519 lorentz_index = ['X', 'Y', 'Z', 'T'] +520 +521 res = [] +522 +523 if name == "TT": +524 for i in range(4): +525 for j in range(i + 1, 4): +526 res.append(("Sigma" + lorentz_index[i] + lorentz_index[j], "Sigma" + lorentz_index[i] + lorentz_index[j])) +527 return res +528 +529 if name == "TTtilde": +530 for i in range(4): +531 for j in range(i + 1, 4): +532 for k in range(4): +533 for o in range(k + 1, 4): +534 fac = epsilon_tensor_rank4(i, j, k, o) +535 if not np.isclose(fac, 0.0): +536 res.append(("Sigma" + lorentz_index[i] + lorentz_index[j], "Sigma" + lorentz_index[k] + lorentz_index[o])) +537 return res +538 +539 assert len(name) == 2 +540 +541 if 'S' in name or 'P' in name: +542 if not set(name) <= set(['S', 'P']): +543 raise Exception("'" + name + "' is not a Lorentz scalar") +544 +545 g_names = {'S': 'Identity', +546 'P': 'Gamma5'} +547 +548 res.append((g_names[name[0]], g_names[name[1]])) +549 +550 else: +551 if not set(name) <= set(['V', 'A']): +552 raise Exception("'" + name + "' is not a Lorentz scalar") +553 +554 for ind in lorentz_index: +555 res.append(('Gamma' + ind + (name[0] == 'A') * 'Gamma5', +556 'Gamma' + ind + (name[1] == 'A') * 'Gamma5')) +557 +558 return res @@ -603,72 +673,72 @@ -
     57def read_meson_hd5(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):
    - 58    r'''Read hadrons meson hdf5 file and extract the meson labeled 'meson'
    - 59
    - 60    Parameters
    - 61    -----------------
    - 62    path : str
    - 63        path to the files to read
    - 64    filestem : str
    - 65        namestem of the files to read
    - 66    ens_id : str
    - 67        name of the ensemble, required for internal bookkeeping
    - 68    meson : str
    - 69        label of the meson to be extracted, standard value meson_0 which
    - 70        corresponds to the pseudoscalar pseudoscalar two-point function.
    - 71    gammas : tuple of strings
    - 72        Instrad of a meson label one can also provide a tuple of two strings
    - 73        indicating the gamma matrices at source and sink.
    - 74        ("Gamma5", "Gamma5") corresponds to the pseudoscalar pseudoscalar
    - 75        two-point function. The gammas argument dominateds over meson.
    - 76    idl : range
    - 77        If specified only configurations in the given range are read in.
    - 78
    - 79    Returns
    - 80    -------
    - 81    corr : Corr
    - 82        Correlator of the source sink combination in question.
    - 83    '''
    - 84
    - 85    files, idx = _get_files(path, filestem, idl)
    - 86
    - 87    tree = meson.rsplit('_')[0]
    - 88    if gammas is not None:
    - 89        h5file = h5py.File(path + '/' + files[0], "r")
    - 90        found_meson = None
    - 91        for key in h5file[tree].keys():
    - 92            if gammas[0] == h5file[tree][key].attrs["gamma_snk"][0].decode() and h5file[tree][key].attrs["gamma_src"][0].decode() == gammas[1]:
    - 93                found_meson = key
    - 94                break
    - 95        h5file.close()
    - 96        if found_meson:
    - 97            meson = found_meson
    - 98        else:
    - 99            raise Exception("Source Sink combination " + str(gammas) + " not found.")
    -100
    -101    corr_data = []
    -102    infos = []
    -103    for hd5_file in files:
    -104        h5file = h5py.File(path + '/' + hd5_file, "r")
    -105        if not tree + '/' + meson in h5file:
    -106            raise Exception("Entry '" + meson + "' not contained in the files.")
    -107        raw_data = h5file[tree + '/' + meson + '/corr']
    -108        real_data = raw_data[:]["re"].astype(np.double)
    -109        corr_data.append(real_data)
    -110        if not infos:
    -111            for k, i in h5file[tree + '/' + meson].attrs.items():
    -112                infos.append(k + ': ' + i[0].decode())
    -113        h5file.close()
    -114    corr_data = np.array(corr_data)
    -115
    -116    l_obs = []
    -117    for c in corr_data.T:
    -118        l_obs.append(Obs([c], [ens_id], idl=[idx]))
    -119
    -120    corr = Corr(l_obs)
    -121    corr.tag = r", ".join(infos)
    -122    return corr
    +            
     58def read_meson_hd5(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):
    + 59    r'''Read hadrons meson hdf5 file and extract the meson labeled 'meson'
    + 60
    + 61    Parameters
    + 62    -----------------
    + 63    path : str
    + 64        path to the files to read
    + 65    filestem : str
    + 66        namestem of the files to read
    + 67    ens_id : str
    + 68        name of the ensemble, required for internal bookkeeping
    + 69    meson : str
    + 70        label of the meson to be extracted, standard value meson_0 which
    + 71        corresponds to the pseudoscalar pseudoscalar two-point function.
    + 72    gammas : tuple of strings
    + 73        Instrad of a meson label one can also provide a tuple of two strings
    + 74        indicating the gamma matrices at source and sink.
    + 75        ("Gamma5", "Gamma5") corresponds to the pseudoscalar pseudoscalar
    + 76        two-point function. The gammas argument dominateds over meson.
    + 77    idl : range
    + 78        If specified only configurations in the given range are read in.
    + 79
    + 80    Returns
    + 81    -------
    + 82    corr : Corr
    + 83        Correlator of the source sink combination in question.
    + 84    '''
    + 85
    + 86    files, idx = _get_files(path, filestem, idl)
    + 87
    + 88    tree = meson.rsplit('_')[0]
    + 89    if gammas is not None:
    + 90        h5file = h5py.File(path + '/' + files[0], "r")
    + 91        found_meson = None
    + 92        for key in h5file[tree].keys():
    + 93            if gammas[0] == h5file[tree][key].attrs["gamma_snk"][0].decode() and h5file[tree][key].attrs["gamma_src"][0].decode() == gammas[1]:
    + 94                found_meson = key
    + 95                break
    + 96        h5file.close()
    + 97        if found_meson:
    + 98            meson = found_meson
    + 99        else:
    +100            raise Exception("Source Sink combination " + str(gammas) + " not found.")
    +101
    +102    corr_data = []
    +103    infos = []
    +104    for hd5_file in files:
    +105        h5file = h5py.File(path + '/' + hd5_file, "r")
    +106        if not tree + '/' + meson in h5file:
    +107            raise Exception("Entry '" + meson + "' not contained in the files.")
    +108        raw_data = h5file[tree + '/' + meson + '/corr']
    +109        real_data = raw_data[:]["re"].astype(np.double)
    +110        corr_data.append(real_data)
    +111        if not infos:
    +112            for k, i in h5file[tree + '/' + meson].attrs.items():
    +113                infos.append(k + ': ' + i[0].decode())
    +114        h5file.close()
    +115    corr_data = np.array(corr_data)
    +116
    +117    l_obs = []
    +118    for c in corr_data.T:
    +119        l_obs.append(Obs([c], [ens_id], idl=[idx]))
    +120
    +121    corr = Corr(l_obs)
    +122    corr.tag = r", ".join(infos)
    +123    return corr
     
    @@ -704,6 +774,92 @@ Correlator of the source sink combination in question.
    + +
    + +
    + + def + extract_t0_hd5( path, filestem, ens_id, obs='Clover energy density', fit_range=5, idl=None, **kwargs): + + + +
    + +
    144def extract_t0_hd5(path, filestem, ens_id, obs='Clover energy density', fit_range=5, idl=None, **kwargs):
    +145    r'''Read hadrons FlowObservables hdf5 file and extract t0
    +146
    +147    Parameters
    +148    -----------------
    +149    path : str
    +150        path to the files to read
    +151    filestem : str
    +152        namestem of the files to read
    +153    ens_id : str
    +154        name of the ensemble, required for internal bookkeeping
    +155    obs : str
    +156        label of the observable from which t0 should be extracted.
    +157        Options: 'Clover energy density' and 'Plaquette energy density'
    +158    fit_range : int
    +159        Number of data points left and right of the zero
    +160        crossing to be included in the linear fit. (Default: 5)
    +161    idl : range
    +162        If specified only configurations in the given range are read in.
    +163    plot_fit : bool
    +164        If true, the fit for the extraction of t0 is shown together with the data.
    +165    '''
    +166
    +167    files, idx = _get_files(path, filestem, idl)
    +168    tree = "FlowObservables"
    +169
    +170    h5file = h5py.File(path + '/' + files[0], "r")
    +171    obs_key = None
    +172    for key in h5file[tree].keys():
    +173        if obs == h5file[tree][key].attrs["description"][0].decode():
    +174            obs_key = key
    +175            break
    +176    h5file.close()
    +177    if obs_key is None:
    +178        raise Exception(f"Observable {obs} not found.")
    +179
    +180    corr_data = _extract_real_arrays(path, files, tree, ["FlowObservables_0", obs_key])
    +181
    +182    if not np.allclose(corr_data["FlowObservables_0"][0], corr_data["FlowObservables_0"][:]):
    +183        raise Exception("Not all flow times were equal.")
    +184
    +185    t2E_dict = {}
    +186    for t2, dat in zip(corr_data["FlowObservables_0"][0], corr_data[obs_key].T):
    +187        t2E_dict[t2] = Obs([dat], [ens_id], idl=[idx]) - 0.3
    +188
    +189    return fit_t0(t2E_dict, fit_range, plot_fit=kwargs.get('plot_fit'))
    +
    + + +

    Read hadrons FlowObservables hdf5 file and extract t0

    + +
    Parameters
    + +
      +
    • path (str): +path to the files to read
    • +
    • filestem (str): +namestem of the files to read
    • +
    • ens_id (str): +name of the ensemble, required for internal bookkeeping
    • +
    • obs (str): +label of the observable from which t0 should be extracted. +Options: 'Clover energy density' and 'Plaquette energy density'
    • +
    • fit_range (int): +Number of data points left and right of the zero +crossing to be included in the linear fit. (Default: 5)
    • +
    • idl (range): +If specified only configurations in the given range are read in.
    • +
    • plot_fit (bool): +If true, the fit for the extraction of t0 is shown together with the data.
    • +
    +
    + +
    @@ -716,101 +872,101 @@ Correlator of the source sink combination in question. -
    125def read_DistillationContraction_hd5(path, ens_id, diagrams=["direct"], idl=None):
    -126    """Read hadrons DistillationContraction hdf5 files in given directory structure
    -127
    -128    Parameters
    -129    -----------------
    -130    path : str
    -131        path to the directories to read
    -132    ens_id : str
    -133        name of the ensemble, required for internal bookkeeping
    -134    diagrams : list
    -135        List of strings of the diagrams to extract, e.g. ["direct", "box", "cross"].
    -136    idl : range
    -137        If specified only configurations in the given range are read in.
    -138
    -139    Returns
    -140    -------
    -141    result : dict
    -142        extracted DistillationContration data
    -143    """
    -144
    -145    res_dict = {}
    -146
    -147    directories, idx = _get_files(path, "data", idl)
    -148
    -149    explore_path = Path(path + "/" + directories[0])
    -150
    -151    for explore_file in explore_path.iterdir():
    -152        if explore_file.is_file():
    -153            stem = explore_file.with_suffix("").with_suffix("").as_posix().split("/")[-1]
    -154        else:
    -155            continue
    -156
    -157        file_list = []
    -158        for dir in directories:
    -159            tmp_path = Path(path + "/" + dir)
    -160            file_list.append((tmp_path / stem).as_posix() + tmp_path.suffix + ".h5")
    -161
    -162        corr_data = {}
    -163
    -164        for diagram in diagrams:
    -165            corr_data[diagram] = []
    -166
    -167        try:
    -168            for n_file, (hd5_file, n_traj) in enumerate(zip(file_list, list(idx))):
    -169                h5file = h5py.File(hd5_file)
    -170
    -171                if n_file == 0:
    -172                    if h5file["DistillationContraction/Metadata"].attrs.get("TimeSources")[0].decode() != "0...":
    -173                        raise Exception("Routine is only implemented for files containing inversions on all timeslices.")
    -174
    -175                    Nt = h5file["DistillationContraction/Metadata"].attrs.get("Nt")[0]
    -176
    -177                    identifier = []
    -178                    for in_file in range(len(h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.keys()) - 1):
    -179                        encoded_info = h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.get("DmfInputFiles_" + str(in_file))
    -180                        full_info = encoded_info[0].decode().split("/")[-1].replace(".h5", "").split("_")
    -181                        my_tuple = (full_info[0], full_info[1][1:], full_info[2], full_info[3])
    -182                        identifier.append(my_tuple)
    -183                    identifier = tuple(identifier)
    -184                    # "DistillationContraction/Metadata/DmfSuffix" contains info about different quarks, irrelevant in the SU(3) case.
    -185
    -186                for diagram in diagrams:
    -187
    -188                    if diagram == "triangle" and "Identity" not in str(identifier):
    -189                        part = "im"
    -190                    else:
    -191                        part = "re"
    -192
    -193                    real_data = np.zeros(Nt)
    -194                    for x0 in range(Nt):
    -195                        raw_data = h5file["DistillationContraction/Correlators/" + diagram + "/" + str(x0)][:][part].astype(np.double)
    -196                        real_data += np.roll(raw_data, -x0)
    -197                    real_data /= Nt
    -198
    -199                    corr_data[diagram].append(real_data)
    -200                h5file.close()
    -201
    -202            res_dict[str(identifier)] = {}
    -203
    -204            for diagram in diagrams:
    +            
    192def read_DistillationContraction_hd5(path, ens_id, diagrams=["direct"], idl=None):
    +193    """Read hadrons DistillationContraction hdf5 files in given directory structure
    +194
    +195    Parameters
    +196    -----------------
    +197    path : str
    +198        path to the directories to read
    +199    ens_id : str
    +200        name of the ensemble, required for internal bookkeeping
    +201    diagrams : list
    +202        List of strings of the diagrams to extract, e.g. ["direct", "box", "cross"].
    +203    idl : range
    +204        If specified only configurations in the given range are read in.
     205
    -206                tmp_data = np.array(corr_data[diagram])
    -207
    -208                l_obs = []
    -209                for c in tmp_data.T:
    -210                    l_obs.append(Obs([c], [ens_id], idl=[idx]))
    +206    Returns
    +207    -------
    +208    result : dict
    +209        extracted DistillationContration data
    +210    """
     211
    -212                corr = Corr(l_obs)
    -213                corr.tag = str(identifier)
    -214
    -215                res_dict[str(identifier)][diagram] = corr
    -216        except FileNotFoundError:
    -217            print("Skip", stem)
    -218
    -219    return res_dict
    +212    res_dict = {}
    +213
    +214    directories, idx = _get_files(path, "data", idl)
    +215
    +216    explore_path = Path(path + "/" + directories[0])
    +217
    +218    for explore_file in explore_path.iterdir():
    +219        if explore_file.is_file():
    +220            stem = explore_file.with_suffix("").with_suffix("").as_posix().split("/")[-1]
    +221        else:
    +222            continue
    +223
    +224        file_list = []
    +225        for dir in directories:
    +226            tmp_path = Path(path + "/" + dir)
    +227            file_list.append((tmp_path / stem).as_posix() + tmp_path.suffix + ".h5")
    +228
    +229        corr_data = {}
    +230
    +231        for diagram in diagrams:
    +232            corr_data[diagram] = []
    +233
    +234        try:
    +235            for n_file, (hd5_file, n_traj) in enumerate(zip(file_list, list(idx))):
    +236                h5file = h5py.File(hd5_file)
    +237
    +238                if n_file == 0:
    +239                    if h5file["DistillationContraction/Metadata"].attrs.get("TimeSources")[0].decode() != "0...":
    +240                        raise Exception("Routine is only implemented for files containing inversions on all timeslices.")
    +241
    +242                    Nt = h5file["DistillationContraction/Metadata"].attrs.get("Nt")[0]
    +243
    +244                    identifier = []
    +245                    for in_file in range(len(h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.keys()) - 1):
    +246                        encoded_info = h5file["DistillationContraction/Metadata/DmfInputFiles"].attrs.get("DmfInputFiles_" + str(in_file))
    +247                        full_info = encoded_info[0].decode().split("/")[-1].replace(".h5", "").split("_")
    +248                        my_tuple = (full_info[0], full_info[1][1:], full_info[2], full_info[3])
    +249                        identifier.append(my_tuple)
    +250                    identifier = tuple(identifier)
    +251                    # "DistillationContraction/Metadata/DmfSuffix" contains info about different quarks, irrelevant in the SU(3) case.
    +252
    +253                for diagram in diagrams:
    +254
    +255                    if diagram == "triangle" and "Identity" not in str(identifier):
    +256                        part = "im"
    +257                    else:
    +258                        part = "re"
    +259
    +260                    real_data = np.zeros(Nt)
    +261                    for x0 in range(Nt):
    +262                        raw_data = h5file["DistillationContraction/Correlators/" + diagram + "/" + str(x0)][:][part].astype(np.double)
    +263                        real_data += np.roll(raw_data, -x0)
    +264                    real_data /= Nt
    +265
    +266                    corr_data[diagram].append(real_data)
    +267                h5file.close()
    +268
    +269            res_dict[str(identifier)] = {}
    +270
    +271            for diagram in diagrams:
    +272
    +273                tmp_data = np.array(corr_data[diagram])
    +274
    +275                l_obs = []
    +276                for c in tmp_data.T:
    +277                    l_obs.append(Obs([c], [ens_id], idl=[idx]))
    +278
    +279                corr = Corr(l_obs)
    +280                corr.tag = str(identifier)
    +281
    +282                res_dict[str(identifier)][diagram] = corr
    +283        except FileNotFoundError:
    +284            print("Skip", stem)
    +285
    +286    return res_dict
     
    @@ -850,44 +1006,44 @@ extracted DistillationContration data
    -
    222class Npr_matrix(np.ndarray):
    -223
    -224    def __new__(cls, input_array, mom_in=None, mom_out=None):
    -225        obj = np.asarray(input_array).view(cls)
    -226        obj.mom_in = mom_in
    -227        obj.mom_out = mom_out
    -228        return obj
    -229
    -230    @property
    -231    def g5H(self):
    -232        """Gamma_5 hermitean conjugate
    -233
    -234        Uses the fact that the propagator is gamma5 hermitean, so just the
    -235        in and out momenta of the propagator are exchanged.
    -236        """
    -237        return Npr_matrix(self,
    -238                          mom_in=self.mom_out,
    -239                          mom_out=self.mom_in)
    -240
    -241    def _propagate_mom(self, other, name):
    -242        s_mom = getattr(self, name, None)
    -243        o_mom = getattr(other, name, None)
    -244        if s_mom is not None and o_mom is not None:
    -245            if not np.allclose(s_mom, o_mom):
    -246                raise Exception(name + ' does not match.')
    -247        return o_mom if o_mom is not None else s_mom
    -248
    -249    def __matmul__(self, other):
    -250        return self.__new__(Npr_matrix,
    -251                            super().__matmul__(other),
    -252                            self._propagate_mom(other, 'mom_in'),
    -253                            self._propagate_mom(other, 'mom_out'))
    -254
    -255    def __array_finalize__(self, obj):
    -256        if obj is None:
    -257            return
    -258        self.mom_in = getattr(obj, 'mom_in', None)
    -259        self.mom_out = getattr(obj, 'mom_out', None)
    +            
    289class Npr_matrix(np.ndarray):
    +290
    +291    def __new__(cls, input_array, mom_in=None, mom_out=None):
    +292        obj = np.asarray(input_array).view(cls)
    +293        obj.mom_in = mom_in
    +294        obj.mom_out = mom_out
    +295        return obj
    +296
    +297    @property
    +298    def g5H(self):
    +299        """Gamma_5 hermitean conjugate
    +300
    +301        Uses the fact that the propagator is gamma5 hermitean, so just the
    +302        in and out momenta of the propagator are exchanged.
    +303        """
    +304        return Npr_matrix(self,
    +305                          mom_in=self.mom_out,
    +306                          mom_out=self.mom_in)
    +307
    +308    def _propagate_mom(self, other, name):
    +309        s_mom = getattr(self, name, None)
    +310        o_mom = getattr(other, name, None)
    +311        if s_mom is not None and o_mom is not None:
    +312            if not np.allclose(s_mom, o_mom):
    +313                raise Exception(name + ' does not match.')
    +314        return o_mom if o_mom is not None else s_mom
    +315
    +316    def __matmul__(self, other):
    +317        return self.__new__(Npr_matrix,
    +318                            super().__matmul__(other),
    +319                            self._propagate_mom(other, 'mom_in'),
    +320                            self._propagate_mom(other, 'mom_out'))
    +321
    +322    def __array_finalize__(self, obj):
    +323        if obj is None:
    +324            return
    +325        self.mom_in = getattr(obj, 'mom_in', None)
    +326        self.mom_out = getattr(obj, 'mom_out', None)
     
    @@ -1130,49 +1286,49 @@ in and out momenta of the propagator are exchanged.

    -
    262def read_ExternalLeg_hd5(path, filestem, ens_id, idl=None):
    -263    """Read hadrons ExternalLeg hdf5 file and output an array of CObs
    -264
    -265    Parameters
    -266    ----------
    -267    path : str
    -268        path to the files to read
    -269    filestem : str
    -270        namestem of the files to read
    -271    ens_id : str
    -272        name of the ensemble, required for internal bookkeeping
    -273    idl : range
    -274        If specified only configurations in the given range are read in.
    -275
    -276    Returns
    -277    -------
    -278    result : Npr_matrix
    -279        read Cobs-matrix
    -280    """
    -281
    -282    files, idx = _get_files(path, filestem, idl)
    -283
    -284    mom = None
    -285
    -286    corr_data = []
    -287    for hd5_file in files:
    -288        file = h5py.File(path + '/' + hd5_file, "r")
    -289        raw_data = file['ExternalLeg/corr'][0][0].view('complex')
    -290        corr_data.append(raw_data)
    -291        if mom is None:
    -292            mom = np.array(str(file['ExternalLeg/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    -293        file.close()
    -294    corr_data = np.array(corr_data)
    -295
    -296    rolled_array = np.rollaxis(corr_data, 0, 5)
    -297
    -298    matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    -299    for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]):
    -300        real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx])
    -301        imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx])
    -302        matrix[si, sj, ci, cj] = CObs(real, imag)
    -303
    -304    return Npr_matrix(matrix, mom_in=mom)
    +            
    329def read_ExternalLeg_hd5(path, filestem, ens_id, idl=None):
    +330    """Read hadrons ExternalLeg hdf5 file and output an array of CObs
    +331
    +332    Parameters
    +333    ----------
    +334    path : str
    +335        path to the files to read
    +336    filestem : str
    +337        namestem of the files to read
    +338    ens_id : str
    +339        name of the ensemble, required for internal bookkeeping
    +340    idl : range
    +341        If specified only configurations in the given range are read in.
    +342
    +343    Returns
    +344    -------
    +345    result : Npr_matrix
    +346        read Cobs-matrix
    +347    """
    +348
    +349    files, idx = _get_files(path, filestem, idl)
    +350
    +351    mom = None
    +352
    +353    corr_data = []
    +354    for hd5_file in files:
    +355        file = h5py.File(path + '/' + hd5_file, "r")
    +356        raw_data = file['ExternalLeg/corr'][0][0].view('complex')
    +357        corr_data.append(raw_data)
    +358        if mom is None:
    +359            mom = np.array(str(file['ExternalLeg/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    +360        file.close()
    +361    corr_data = np.array(corr_data)
    +362
    +363    rolled_array = np.rollaxis(corr_data, 0, 5)
    +364
    +365    matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    +366    for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]):
    +367        real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx])
    +368        imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx])
    +369        matrix[si, sj, ci, cj] = CObs(real, imag)
    +370
    +371    return Npr_matrix(matrix, mom_in=mom)
     
    @@ -1212,63 +1368,63 @@ read Cobs-matrix
    -
    307def read_Bilinear_hd5(path, filestem, ens_id, idl=None):
    -308    """Read hadrons Bilinear hdf5 file and output an array of CObs
    -309
    -310    Parameters
    -311    ----------
    -312    path : str
    -313        path to the files to read
    -314    filestem : str
    -315        namestem of the files to read
    -316    ens_id : str
    -317        name of the ensemble, required for internal bookkeeping
    -318    idl : range
    -319        If specified only configurations in the given range are read in.
    -320
    -321    Returns
    -322    -------
    -323    result_dict: dict[Npr_matrix]
    -324        extracted Bilinears
    -325    """
    -326
    -327    files, idx = _get_files(path, filestem, idl)
    -328
    -329    mom_in = None
    -330    mom_out = None
    -331
    -332    corr_data = {}
    -333    for hd5_file in files:
    -334        file = h5py.File(path + '/' + hd5_file, "r")
    -335        for i in range(16):
    -336            name = file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['gamma'][0].decode('UTF-8')
    -337            if name not in corr_data:
    -338                corr_data[name] = []
    -339            raw_data = file['Bilinear/Bilinear_' + str(i) + '/corr'][0][0].view('complex')
    -340            corr_data[name].append(raw_data)
    -341            if mom_in is None:
    -342                mom_in = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    -343            if mom_out is None:
    -344                mom_out = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float)
    -345
    -346        file.close()
    -347
    -348    result_dict = {}
    -349
    -350    for key, data in corr_data.items():
    -351        local_data = np.array(data)
    -352
    -353        rolled_array = np.rollaxis(local_data, 0, 5)
    -354
    -355        matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    -356        for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]):
    -357            real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx])
    -358            imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx])
    -359            matrix[si, sj, ci, cj] = CObs(real, imag)
    -360
    -361        result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out)
    -362
    -363    return result_dict
    +            
    374def read_Bilinear_hd5(path, filestem, ens_id, idl=None):
    +375    """Read hadrons Bilinear hdf5 file and output an array of CObs
    +376
    +377    Parameters
    +378    ----------
    +379    path : str
    +380        path to the files to read
    +381    filestem : str
    +382        namestem of the files to read
    +383    ens_id : str
    +384        name of the ensemble, required for internal bookkeeping
    +385    idl : range
    +386        If specified only configurations in the given range are read in.
    +387
    +388    Returns
    +389    -------
    +390    result_dict: dict[Npr_matrix]
    +391        extracted Bilinears
    +392    """
    +393
    +394    files, idx = _get_files(path, filestem, idl)
    +395
    +396    mom_in = None
    +397    mom_out = None
    +398
    +399    corr_data = {}
    +400    for hd5_file in files:
    +401        file = h5py.File(path + '/' + hd5_file, "r")
    +402        for i in range(16):
    +403            name = file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['gamma'][0].decode('UTF-8')
    +404            if name not in corr_data:
    +405                corr_data[name] = []
    +406            raw_data = file['Bilinear/Bilinear_' + str(i) + '/corr'][0][0].view('complex')
    +407            corr_data[name].append(raw_data)
    +408            if mom_in is None:
    +409                mom_in = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    +410            if mom_out is None:
    +411                mom_out = np.array(str(file['Bilinear/Bilinear_' + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float)
    +412
    +413        file.close()
    +414
    +415    result_dict = {}
    +416
    +417    for key, data in corr_data.items():
    +418        local_data = np.array(data)
    +419
    +420        rolled_array = np.rollaxis(local_data, 0, 5)
    +421
    +422        matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    +423        for si, sj, ci, cj in np.ndindex(rolled_array.shape[:-1]):
    +424            real = Obs([rolled_array[si, sj, ci, cj].real], [ens_id], idl=[idx])
    +425            imag = Obs([rolled_array[si, sj, ci, cj].imag], [ens_id], idl=[idx])
    +426            matrix[si, sj, ci, cj] = CObs(real, imag)
    +427
    +428        result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out)
    +429
    +430    return result_dict
     
    @@ -1308,90 +1464,90 @@ extracted Bilinears
    -
    366def read_Fourquark_hd5(path, filestem, ens_id, idl=None, vertices=["VA", "AV"]):
    -367    """Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs
    -368
    -369    Parameters
    -370    ----------
    -371    path : str
    -372        path to the files to read
    -373    filestem : str
    -374        namestem of the files to read
    -375    ens_id : str
    -376        name of the ensemble, required for internal bookkeeping
    -377    idl : range
    -378        If specified only configurations in the given range are read in.
    -379    vertices : list
    -380        Vertex functions to be extracted.
    -381
    -382    Returns
    -383    -------
    -384    result_dict : dict
    -385        extracted fourquark matrizes
    -386    """
    -387
    -388    files, idx = _get_files(path, filestem, idl)
    -389
    -390    mom_in = None
    -391    mom_out = None
    -392
    -393    vertex_names = []
    -394    for vertex in vertices:
    -395        vertex_names += _get_lorentz_names(vertex)
    -396
    -397    corr_data = {}
    -398
    -399    tree = 'FourQuarkFullyConnected/FourQuarkFullyConnected_'
    -400
    -401    for hd5_file in files:
    -402        file = h5py.File(path + '/' + hd5_file, "r")
    -403
    -404        for i in range(32):
    -405            name = (file[tree + str(i) + '/info'].attrs['gammaA'][0].decode('UTF-8'), file[tree + str(i) + '/info'].attrs['gammaB'][0].decode('UTF-8'))
    -406            if name in vertex_names:
    -407                if name not in corr_data:
    -408                    corr_data[name] = []
    -409                raw_data = file[tree + str(i) + '/corr'][0][0].view('complex')
    -410                corr_data[name].append(raw_data)
    -411                if mom_in is None:
    -412                    mom_in = np.array(str(file[tree + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    -413                if mom_out is None:
    -414                    mom_out = np.array(str(file[tree + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float)
    -415
    -416        file.close()
    -417
    -418    intermediate_dict = {}
    -419
    -420    for vertex in vertices:
    -421        lorentz_names = _get_lorentz_names(vertex)
    -422        for v_name in lorentz_names:
    -423            if v_name in [('SigmaXY', 'SigmaZT'),
    -424                          ('SigmaXT', 'SigmaYZ'),
    -425                          ('SigmaYZ', 'SigmaXT'),
    -426                          ('SigmaZT', 'SigmaXY')]:
    -427                sign = -1
    -428            else:
    -429                sign = 1
    -430            if vertex not in intermediate_dict:
    -431                intermediate_dict[vertex] = sign * np.array(corr_data[v_name])
    -432            else:
    -433                intermediate_dict[vertex] += sign * np.array(corr_data[v_name])
    -434
    -435    result_dict = {}
    -436
    -437    for key, data in intermediate_dict.items():
    -438
    -439        rolled_array = np.moveaxis(data, 0, 8)
    -440
    -441        matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    -442        for index in np.ndindex(rolled_array.shape[:-1]):
    -443            real = Obs([rolled_array[index].real], [ens_id], idl=[idx])
    -444            imag = Obs([rolled_array[index].imag], [ens_id], idl=[idx])
    -445            matrix[index] = CObs(real, imag)
    -446
    -447        result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out)
    +            
    433def read_Fourquark_hd5(path, filestem, ens_id, idl=None, vertices=["VA", "AV"]):
    +434    """Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs
    +435
    +436    Parameters
    +437    ----------
    +438    path : str
    +439        path to the files to read
    +440    filestem : str
    +441        namestem of the files to read
    +442    ens_id : str
    +443        name of the ensemble, required for internal bookkeeping
    +444    idl : range
    +445        If specified only configurations in the given range are read in.
    +446    vertices : list
    +447        Vertex functions to be extracted.
     448
    -449    return result_dict
    +449    Returns
    +450    -------
    +451    result_dict : dict
    +452        extracted fourquark matrizes
    +453    """
    +454
    +455    files, idx = _get_files(path, filestem, idl)
    +456
    +457    mom_in = None
    +458    mom_out = None
    +459
    +460    vertex_names = []
    +461    for vertex in vertices:
    +462        vertex_names += _get_lorentz_names(vertex)
    +463
    +464    corr_data = {}
    +465
    +466    tree = 'FourQuarkFullyConnected/FourQuarkFullyConnected_'
    +467
    +468    for hd5_file in files:
    +469        file = h5py.File(path + '/' + hd5_file, "r")
    +470
    +471        for i in range(32):
    +472            name = (file[tree + str(i) + '/info'].attrs['gammaA'][0].decode('UTF-8'), file[tree + str(i) + '/info'].attrs['gammaB'][0].decode('UTF-8'))
    +473            if name in vertex_names:
    +474                if name not in corr_data:
    +475                    corr_data[name] = []
    +476                raw_data = file[tree + str(i) + '/corr'][0][0].view('complex')
    +477                corr_data[name].append(raw_data)
    +478                if mom_in is None:
    +479                    mom_in = np.array(str(file[tree + str(i) + '/info'].attrs['pIn'])[3:-2].strip().split(), dtype=float)
    +480                if mom_out is None:
    +481                    mom_out = np.array(str(file[tree + str(i) + '/info'].attrs['pOut'])[3:-2].strip().split(), dtype=float)
    +482
    +483        file.close()
    +484
    +485    intermediate_dict = {}
    +486
    +487    for vertex in vertices:
    +488        lorentz_names = _get_lorentz_names(vertex)
    +489        for v_name in lorentz_names:
    +490            if v_name in [('SigmaXY', 'SigmaZT'),
    +491                          ('SigmaXT', 'SigmaYZ'),
    +492                          ('SigmaYZ', 'SigmaXT'),
    +493                          ('SigmaZT', 'SigmaXY')]:
    +494                sign = -1
    +495            else:
    +496                sign = 1
    +497            if vertex not in intermediate_dict:
    +498                intermediate_dict[vertex] = sign * np.array(corr_data[v_name])
    +499            else:
    +500                intermediate_dict[vertex] += sign * np.array(corr_data[v_name])
    +501
    +502    result_dict = {}
    +503
    +504    for key, data in intermediate_dict.items():
    +505
    +506        rolled_array = np.moveaxis(data, 0, 8)
    +507
    +508        matrix = np.empty((rolled_array.shape[:-1]), dtype=object)
    +509        for index in np.ndindex(rolled_array.shape[:-1]):
    +510            real = Obs([rolled_array[index].real], [ens_id], idl=[idx])
    +511            imag = Obs([rolled_array[index].imag], [ens_id], idl=[idx])
    +512            matrix[index] = CObs(real, imag)
    +513
    +514        result_dict[key] = Npr_matrix(matrix, mom_in=mom_in, mom_out=mom_out)
    +515
    +516    return result_dict
     
    diff --git a/docs/pyerrors/input/json.html b/docs/pyerrors/input/json.html index d2ce8fec..93a60603 100644 --- a/docs/pyerrors/input/json.html +++ b/docs/pyerrors/input/json.html @@ -3,7 +3,7 @@ - + pyerrors.input.json API documentation diff --git a/docs/pyerrors/input/misc.html b/docs/pyerrors/input/misc.html index 529b4d49..1e1873f9 100644 --- a/docs/pyerrors/input/misc.html +++ b/docs/pyerrors/input/misc.html @@ -3,7 +3,7 @@ - + pyerrors.input.misc API documentation @@ -52,6 +52,9 @@

    API Documentation

      +
    • + fit_t0 +
    • read_pbp
    • @@ -81,132 +84,246 @@ 3import re 4import struct 5import numpy as np # Thinly-wrapped numpy - 6from ..obs import Obs - 7 - 8 - 9def read_pbp(path, prefix, **kwargs): - 10 """Read pbp format from given folder structure. + 6import matplotlib.pyplot as plt + 7from matplotlib import gridspec + 8from ..obs import Obs + 9from ..fits import fit_lin + 10 11 - 12 Parameters - 13 ---------- - 14 r_start : list - 15 list which contains the first config to be read for each replicum - 16 r_stop : list - 17 list which contains the last config to be read for each replicum - 18 - 19 Returns - 20 ------- - 21 result : list[Obs] - 22 list of observables read - 23 """ - 24 - 25 ls = [] - 26 for (dirpath, dirnames, filenames) in os.walk(path): - 27 ls.extend(filenames) - 28 break - 29 - 30 if not ls: - 31 raise Exception('Error, directory not found') - 32 - 33 # Exclude files with different names - 34 for exc in ls: - 35 if not fnmatch.fnmatch(exc, prefix + '*.dat'): - 36 ls = list(set(ls) - set([exc])) - 37 if len(ls) > 1: - 38 ls.sort(key=lambda x: int(re.findall(r'\d+', x[len(prefix):])[0])) - 39 replica = len(ls) - 40 - 41 if 'r_start' in kwargs: - 42 r_start = kwargs.get('r_start') - 43 if len(r_start) != replica: - 44 raise Exception('r_start does not match number of replicas') - 45 # Adjust Configuration numbering to python index - 46 r_start = [o - 1 if o else None for o in r_start] - 47 else: - 48 r_start = [None] * replica - 49 - 50 if 'r_stop' in kwargs: - 51 r_stop = kwargs.get('r_stop') - 52 if len(r_stop) != replica: - 53 raise Exception('r_stop does not match number of replicas') - 54 else: - 55 r_stop = [None] * replica - 56 - 57 print(r'Read <bar{psi}\psi> from', prefix[:-1], ',', replica, 'replica', end='') + 12def fit_t0(t2E_dict, fit_range, plot_fit=False): + 13 zero_crossing = np.argmax(np.array( + 14 [o.value for o in t2E_dict.values()]) > 0.0) + 15 + 16 x = list(t2E_dict.keys())[zero_crossing - fit_range: + 17 zero_crossing + fit_range] + 18 y = list(t2E_dict.values())[zero_crossing - fit_range: + 19 zero_crossing + fit_range] + 20 [o.gamma_method() for o in y] + 21 + 22 fit_result = fit_lin(x, y) + 23 + 24 if plot_fit is True: + 25 plt.figure() + 26 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) + 27 ax0 = plt.subplot(gs[0]) + 28 xmore = list(t2E_dict.keys())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2] + 29 ymore = list(t2E_dict.values())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2] + 30 [o.gamma_method() for o in ymore] + 31 ax0.errorbar(xmore, [yi.value for yi in ymore], yerr=[yi.dvalue for yi in ymore], fmt='x') + 32 xplot = np.linspace(np.min(x), np.max(x)) + 33 yplot = [fit_result[0] + fit_result[1] * xi for xi in xplot] + 34 [yi.gamma_method() for yi in yplot] + 35 ax0.fill_between(xplot, y1=[yi.value - yi.dvalue for yi in yplot], y2=[yi.value + yi.dvalue for yi in yplot]) + 36 retval = (-fit_result[0] / fit_result[1]) + 37 retval.gamma_method() + 38 ylim = ax0.get_ylim() + 39 ax0.fill_betweenx(ylim, x1=retval.value - retval.dvalue, x2=retval.value + retval.dvalue, color='gray', alpha=0.4) + 40 ax0.set_ylim(ylim) + 41 ax0.set_ylabel(r'$t^2 \langle E(t) \rangle - 0.3 $') + 42 xlim = ax0.get_xlim() + 43 + 44 fit_res = [fit_result[0] + fit_result[1] * xi for xi in x] + 45 residuals = (np.asarray([o.value for o in y]) - [o.value for o in fit_res]) / np.asarray([o.dvalue for o in y]) + 46 ax1 = plt.subplot(gs[1]) + 47 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) + 48 ax1.tick_params(direction='out') + 49 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) + 50 ax1.axhline(y=0.0, ls='--', color='k') + 51 ax1.fill_between(xlim, -1.0, 1.0, alpha=0.1, facecolor='k') + 52 ax1.set_xlim(xlim) + 53 ax1.set_ylabel('Residuals') + 54 ax1.set_xlabel(r'$t/a^2$') + 55 + 56 plt.draw() + 57 return -fit_result[0] / fit_result[1] 58 - 59 print_err = 0 - 60 if 'print_err' in kwargs: - 61 print_err = 1 - 62 print() - 63 - 64 deltas = [] - 65 - 66 for rep in range(replica): - 67 tmp_array = [] - 68 with open(path + '/' + ls[rep], 'rb') as fp: + 59 + 60def read_pbp(path, prefix, **kwargs): + 61 """Read pbp format from given folder structure. + 62 + 63 Parameters + 64 ---------- + 65 r_start : list + 66 list which contains the first config to be read for each replicum + 67 r_stop : list + 68 list which contains the last config to be read for each replicum 69 - 70 t = fp.read(4) # number of reweighting factors - 71 if rep == 0: - 72 nrw = struct.unpack('i', t)[0] - 73 for k in range(nrw): - 74 deltas.append([]) - 75 else: - 76 if nrw != struct.unpack('i', t)[0]: - 77 raise Exception('Error: different number of factors for replicum', rep) - 78 - 79 for k in range(nrw): - 80 tmp_array.append([]) - 81 - 82 # This block is necessary for openQCD1.6 ms1 files - 83 nfct = [] - 84 for i in range(nrw): - 85 t = fp.read(4) - 86 nfct.append(struct.unpack('i', t)[0]) - 87 print('nfct: ', nfct) # Hasenbusch factor, 1 for rat reweighting - 88 - 89 nsrc = [] - 90 for i in range(nrw): - 91 t = fp.read(4) - 92 nsrc.append(struct.unpack('i', t)[0]) - 93 - 94 # body - 95 while True: - 96 t = fp.read(4) - 97 if len(t) < 4: - 98 break - 99 if print_err: -100 config_no = struct.unpack('i', t) -101 for i in range(nrw): -102 tmp_nfct = 1.0 -103 for j in range(nfct[i]): -104 t = fp.read(8 * nsrc[i]) -105 t = fp.read(8 * nsrc[i]) -106 tmp_rw = struct.unpack('d' * nsrc[i], t) -107 tmp_nfct *= np.mean(np.asarray(tmp_rw)) -108 if print_err: -109 print(config_no, i, j, np.mean(np.asarray(tmp_rw)), np.std(np.asarray(tmp_rw))) -110 print('Sources:', np.asarray(tmp_rw)) -111 print('Partial factor:', tmp_nfct) -112 tmp_array[i].append(tmp_nfct) -113 -114 for k in range(nrw): -115 deltas[k].append(tmp_array[k][r_start[rep]:r_stop[rep]]) + 70 Returns + 71 ------- + 72 result : list[Obs] + 73 list of observables read + 74 """ + 75 + 76 ls = [] + 77 for (dirpath, dirnames, filenames) in os.walk(path): + 78 ls.extend(filenames) + 79 break + 80 + 81 if not ls: + 82 raise Exception('Error, directory not found') + 83 + 84 # Exclude files with different names + 85 for exc in ls: + 86 if not fnmatch.fnmatch(exc, prefix + '*.dat'): + 87 ls = list(set(ls) - set([exc])) + 88 if len(ls) > 1: + 89 ls.sort(key=lambda x: int(re.findall(r'\d+', x[len(prefix):])[0])) + 90 replica = len(ls) + 91 + 92 if 'r_start' in kwargs: + 93 r_start = kwargs.get('r_start') + 94 if len(r_start) != replica: + 95 raise Exception('r_start does not match number of replicas') + 96 # Adjust Configuration numbering to python index + 97 r_start = [o - 1 if o else None for o in r_start] + 98 else: + 99 r_start = [None] * replica +100 +101 if 'r_stop' in kwargs: +102 r_stop = kwargs.get('r_stop') +103 if len(r_stop) != replica: +104 raise Exception('r_stop does not match number of replicas') +105 else: +106 r_stop = [None] * replica +107 +108 print(r'Read <bar{psi}\psi> from', prefix[:-1], ',', replica, 'replica', end='') +109 +110 print_err = 0 +111 if 'print_err' in kwargs: +112 print_err = 1 +113 print() +114 +115 deltas = [] 116 -117 rep_names = [] -118 for entry in ls: -119 truncated_entry = entry.split('.')[0] -120 idx = truncated_entry.index('r') -121 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) -122 print(',', nrw, r'<bar{psi}\psi> with', nsrc, 'sources') -123 result = [] -124 for t in range(nrw): -125 result.append(Obs(deltas[t], rep_names)) -126 -127 return result +117 for rep in range(replica): +118 tmp_array = [] +119 with open(path + '/' + ls[rep], 'rb') as fp: +120 +121 t = fp.read(4) # number of reweighting factors +122 if rep == 0: +123 nrw = struct.unpack('i', t)[0] +124 for k in range(nrw): +125 deltas.append([]) +126 else: +127 if nrw != struct.unpack('i', t)[0]: +128 raise Exception('Error: different number of factors for replicum', rep) +129 +130 for k in range(nrw): +131 tmp_array.append([]) +132 +133 # This block is necessary for openQCD1.6 ms1 files +134 nfct = [] +135 for i in range(nrw): +136 t = fp.read(4) +137 nfct.append(struct.unpack('i', t)[0]) +138 print('nfct: ', nfct) # Hasenbusch factor, 1 for rat reweighting +139 +140 nsrc = [] +141 for i in range(nrw): +142 t = fp.read(4) +143 nsrc.append(struct.unpack('i', t)[0]) +144 +145 # body +146 while True: +147 t = fp.read(4) +148 if len(t) < 4: +149 break +150 if print_err: +151 config_no = struct.unpack('i', t) +152 for i in range(nrw): +153 tmp_nfct = 1.0 +154 for j in range(nfct[i]): +155 t = fp.read(8 * nsrc[i]) +156 t = fp.read(8 * nsrc[i]) +157 tmp_rw = struct.unpack('d' * nsrc[i], t) +158 tmp_nfct *= np.mean(np.asarray(tmp_rw)) +159 if print_err: +160 print(config_no, i, j, np.mean(np.asarray(tmp_rw)), np.std(np.asarray(tmp_rw))) +161 print('Sources:', np.asarray(tmp_rw)) +162 print('Partial factor:', tmp_nfct) +163 tmp_array[i].append(tmp_nfct) +164 +165 for k in range(nrw): +166 deltas[k].append(tmp_array[k][r_start[rep]:r_stop[rep]]) +167 +168 rep_names = [] +169 for entry in ls: +170 truncated_entry = entry.split('.')[0] +171 idx = truncated_entry.index('r') +172 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) +173 print(',', nrw, r'<bar{psi}\psi> with', nsrc, 'sources') +174 result = [] +175 for t in range(nrw): +176 result.append(Obs(deltas[t], rep_names)) +177 +178 return result
    +
    + +
    + + def + fit_t0(t2E_dict, fit_range, plot_fit=False): + + + +
    + +
    13def fit_t0(t2E_dict, fit_range, plot_fit=False):
    +14    zero_crossing = np.argmax(np.array(
    +15        [o.value for o in t2E_dict.values()]) > 0.0)
    +16
    +17    x = list(t2E_dict.keys())[zero_crossing - fit_range:
    +18                              zero_crossing + fit_range]
    +19    y = list(t2E_dict.values())[zero_crossing - fit_range:
    +20                                zero_crossing + fit_range]
    +21    [o.gamma_method() for o in y]
    +22
    +23    fit_result = fit_lin(x, y)
    +24
    +25    if plot_fit is True:
    +26        plt.figure()
    +27        gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0)
    +28        ax0 = plt.subplot(gs[0])
    +29        xmore = list(t2E_dict.keys())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2]
    +30        ymore = list(t2E_dict.values())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2]
    +31        [o.gamma_method() for o in ymore]
    +32        ax0.errorbar(xmore, [yi.value for yi in ymore], yerr=[yi.dvalue for yi in ymore], fmt='x')
    +33        xplot = np.linspace(np.min(x), np.max(x))
    +34        yplot = [fit_result[0] + fit_result[1] * xi for xi in xplot]
    +35        [yi.gamma_method() for yi in yplot]
    +36        ax0.fill_between(xplot, y1=[yi.value - yi.dvalue for yi in yplot], y2=[yi.value + yi.dvalue for yi in yplot])
    +37        retval = (-fit_result[0] / fit_result[1])
    +38        retval.gamma_method()
    +39        ylim = ax0.get_ylim()
    +40        ax0.fill_betweenx(ylim, x1=retval.value - retval.dvalue, x2=retval.value + retval.dvalue, color='gray', alpha=0.4)
    +41        ax0.set_ylim(ylim)
    +42        ax0.set_ylabel(r'$t^2 \langle E(t) \rangle - 0.3 $')
    +43        xlim = ax0.get_xlim()
    +44
    +45        fit_res = [fit_result[0] + fit_result[1] * xi for xi in x]
    +46        residuals = (np.asarray([o.value for o in y]) - [o.value for o in fit_res]) / np.asarray([o.dvalue for o in y])
    +47        ax1 = plt.subplot(gs[1])
    +48        ax1.plot(x, residuals, 'ko', ls='none', markersize=5)
    +49        ax1.tick_params(direction='out')
    +50        ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True)
    +51        ax1.axhline(y=0.0, ls='--', color='k')
    +52        ax1.fill_between(xlim, -1.0, 1.0, alpha=0.1, facecolor='k')
    +53        ax1.set_xlim(xlim)
    +54        ax1.set_ylabel('Residuals')
    +55        ax1.set_xlabel(r'$t/a^2$')
    +56
    +57        plt.draw()
    +58    return -fit_result[0] / fit_result[1]
    +
    + + + + +
    @@ -218,125 +335,125 @@
    -
     10def read_pbp(path, prefix, **kwargs):
    - 11    """Read pbp format from given folder structure.
    - 12
    - 13    Parameters
    - 14    ----------
    - 15    r_start : list
    - 16        list which contains the first config to be read for each replicum
    - 17    r_stop : list
    - 18        list which contains the last config to be read for each replicum
    - 19
    - 20    Returns
    - 21    -------
    - 22    result : list[Obs]
    - 23        list of observables read
    - 24    """
    - 25
    - 26    ls = []
    - 27    for (dirpath, dirnames, filenames) in os.walk(path):
    - 28        ls.extend(filenames)
    - 29        break
    - 30
    - 31    if not ls:
    - 32        raise Exception('Error, directory not found')
    - 33
    - 34    # Exclude files with different names
    - 35    for exc in ls:
    - 36        if not fnmatch.fnmatch(exc, prefix + '*.dat'):
    - 37            ls = list(set(ls) - set([exc]))
    - 38    if len(ls) > 1:
    - 39        ls.sort(key=lambda x: int(re.findall(r'\d+', x[len(prefix):])[0]))
    - 40    replica = len(ls)
    - 41
    - 42    if 'r_start' in kwargs:
    - 43        r_start = kwargs.get('r_start')
    - 44        if len(r_start) != replica:
    - 45            raise Exception('r_start does not match number of replicas')
    - 46        # Adjust Configuration numbering to python index
    - 47        r_start = [o - 1 if o else None for o in r_start]
    - 48    else:
    - 49        r_start = [None] * replica
    - 50
    - 51    if 'r_stop' in kwargs:
    - 52        r_stop = kwargs.get('r_stop')
    - 53        if len(r_stop) != replica:
    - 54            raise Exception('r_stop does not match number of replicas')
    - 55    else:
    - 56        r_stop = [None] * replica
    - 57
    - 58    print(r'Read <bar{psi}\psi> from', prefix[:-1], ',', replica, 'replica', end='')
    - 59
    - 60    print_err = 0
    - 61    if 'print_err' in kwargs:
    - 62        print_err = 1
    - 63        print()
    - 64
    - 65    deltas = []
    - 66
    - 67    for rep in range(replica):
    - 68        tmp_array = []
    - 69        with open(path + '/' + ls[rep], 'rb') as fp:
    +            
     61def read_pbp(path, prefix, **kwargs):
    + 62    """Read pbp format from given folder structure.
    + 63
    + 64    Parameters
    + 65    ----------
    + 66    r_start : list
    + 67        list which contains the first config to be read for each replicum
    + 68    r_stop : list
    + 69        list which contains the last config to be read for each replicum
      70
    - 71            t = fp.read(4)  # number of reweighting factors
    - 72            if rep == 0:
    - 73                nrw = struct.unpack('i', t)[0]
    - 74                for k in range(nrw):
    - 75                    deltas.append([])
    - 76            else:
    - 77                if nrw != struct.unpack('i', t)[0]:
    - 78                    raise Exception('Error: different number of factors for replicum', rep)
    - 79
    - 80            for k in range(nrw):
    - 81                tmp_array.append([])
    - 82
    - 83            # This block is necessary for openQCD1.6 ms1 files
    - 84            nfct = []
    - 85            for i in range(nrw):
    - 86                t = fp.read(4)
    - 87                nfct.append(struct.unpack('i', t)[0])
    - 88            print('nfct: ', nfct)  # Hasenbusch factor, 1 for rat reweighting
    - 89
    - 90            nsrc = []
    - 91            for i in range(nrw):
    - 92                t = fp.read(4)
    - 93                nsrc.append(struct.unpack('i', t)[0])
    - 94
    - 95            # body
    - 96            while True:
    - 97                t = fp.read(4)
    - 98                if len(t) < 4:
    - 99                    break
    -100                if print_err:
    -101                    config_no = struct.unpack('i', t)
    -102                for i in range(nrw):
    -103                    tmp_nfct = 1.0
    -104                    for j in range(nfct[i]):
    -105                        t = fp.read(8 * nsrc[i])
    -106                        t = fp.read(8 * nsrc[i])
    -107                        tmp_rw = struct.unpack('d' * nsrc[i], t)
    -108                        tmp_nfct *= np.mean(np.asarray(tmp_rw))
    -109                        if print_err:
    -110                            print(config_no, i, j, np.mean(np.asarray(tmp_rw)), np.std(np.asarray(tmp_rw)))
    -111                            print('Sources:', np.asarray(tmp_rw))
    -112                            print('Partial factor:', tmp_nfct)
    -113                    tmp_array[i].append(tmp_nfct)
    -114
    -115            for k in range(nrw):
    -116                deltas[k].append(tmp_array[k][r_start[rep]:r_stop[rep]])
    + 71    Returns
    + 72    -------
    + 73    result : list[Obs]
    + 74        list of observables read
    + 75    """
    + 76
    + 77    ls = []
    + 78    for (dirpath, dirnames, filenames) in os.walk(path):
    + 79        ls.extend(filenames)
    + 80        break
    + 81
    + 82    if not ls:
    + 83        raise Exception('Error, directory not found')
    + 84
    + 85    # Exclude files with different names
    + 86    for exc in ls:
    + 87        if not fnmatch.fnmatch(exc, prefix + '*.dat'):
    + 88            ls = list(set(ls) - set([exc]))
    + 89    if len(ls) > 1:
    + 90        ls.sort(key=lambda x: int(re.findall(r'\d+', x[len(prefix):])[0]))
    + 91    replica = len(ls)
    + 92
    + 93    if 'r_start' in kwargs:
    + 94        r_start = kwargs.get('r_start')
    + 95        if len(r_start) != replica:
    + 96            raise Exception('r_start does not match number of replicas')
    + 97        # Adjust Configuration numbering to python index
    + 98        r_start = [o - 1 if o else None for o in r_start]
    + 99    else:
    +100        r_start = [None] * replica
    +101
    +102    if 'r_stop' in kwargs:
    +103        r_stop = kwargs.get('r_stop')
    +104        if len(r_stop) != replica:
    +105            raise Exception('r_stop does not match number of replicas')
    +106    else:
    +107        r_stop = [None] * replica
    +108
    +109    print(r'Read <bar{psi}\psi> from', prefix[:-1], ',', replica, 'replica', end='')
    +110
    +111    print_err = 0
    +112    if 'print_err' in kwargs:
    +113        print_err = 1
    +114        print()
    +115
    +116    deltas = []
     117
    -118    rep_names = []
    -119    for entry in ls:
    -120        truncated_entry = entry.split('.')[0]
    -121        idx = truncated_entry.index('r')
    -122        rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    -123    print(',', nrw, r'<bar{psi}\psi> with', nsrc, 'sources')
    -124    result = []
    -125    for t in range(nrw):
    -126        result.append(Obs(deltas[t], rep_names))
    -127
    -128    return result
    +118    for rep in range(replica):
    +119        tmp_array = []
    +120        with open(path + '/' + ls[rep], 'rb') as fp:
    +121
    +122            t = fp.read(4)  # number of reweighting factors
    +123            if rep == 0:
    +124                nrw = struct.unpack('i', t)[0]
    +125                for k in range(nrw):
    +126                    deltas.append([])
    +127            else:
    +128                if nrw != struct.unpack('i', t)[0]:
    +129                    raise Exception('Error: different number of factors for replicum', rep)
    +130
    +131            for k in range(nrw):
    +132                tmp_array.append([])
    +133
    +134            # This block is necessary for openQCD1.6 ms1 files
    +135            nfct = []
    +136            for i in range(nrw):
    +137                t = fp.read(4)
    +138                nfct.append(struct.unpack('i', t)[0])
    +139            print('nfct: ', nfct)  # Hasenbusch factor, 1 for rat reweighting
    +140
    +141            nsrc = []
    +142            for i in range(nrw):
    +143                t = fp.read(4)
    +144                nsrc.append(struct.unpack('i', t)[0])
    +145
    +146            # body
    +147            while True:
    +148                t = fp.read(4)
    +149                if len(t) < 4:
    +150                    break
    +151                if print_err:
    +152                    config_no = struct.unpack('i', t)
    +153                for i in range(nrw):
    +154                    tmp_nfct = 1.0
    +155                    for j in range(nfct[i]):
    +156                        t = fp.read(8 * nsrc[i])
    +157                        t = fp.read(8 * nsrc[i])
    +158                        tmp_rw = struct.unpack('d' * nsrc[i], t)
    +159                        tmp_nfct *= np.mean(np.asarray(tmp_rw))
    +160                        if print_err:
    +161                            print(config_no, i, j, np.mean(np.asarray(tmp_rw)), np.std(np.asarray(tmp_rw)))
    +162                            print('Sources:', np.asarray(tmp_rw))
    +163                            print('Partial factor:', tmp_nfct)
    +164                    tmp_array[i].append(tmp_nfct)
    +165
    +166            for k in range(nrw):
    +167                deltas[k].append(tmp_array[k][r_start[rep]:r_stop[rep]])
    +168
    +169    rep_names = []
    +170    for entry in ls:
    +171        truncated_entry = entry.split('.')[0]
    +172        idx = truncated_entry.index('r')
    +173        rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    +174    print(',', nrw, r'<bar{psi}\psi> with', nsrc, 'sources')
    +175    result = []
    +176    for t in range(nrw):
    +177        result.append(Obs(deltas[t], rep_names))
    +178
    +179    return result
     
    diff --git a/docs/pyerrors/input/openQCD.html b/docs/pyerrors/input/openQCD.html index a2977331..f5b355d2 100644 --- a/docs/pyerrors/input/openQCD.html +++ b/docs/pyerrors/input/openQCD.html @@ -3,7 +3,7 @@ - + pyerrors.input.openQCD API documentation @@ -99,1197 +99,1151 @@
    3import struct 4import warnings 5import numpy as np # Thinly-wrapped numpy - 6import matplotlib.pyplot as plt - 7from matplotlib import gridspec - 8from ..obs import Obs - 9from ..fits import fit_lin - 10from ..obs import CObs - 11from ..correlators import Corr - 12from .utils import sort_names - 13 - 14 - 15def read_rwms(path, prefix, version='2.0', names=None, **kwargs): - 16 """Read rwms format from given folder structure. Returns a list of length nrw - 17 - 18 Parameters - 19 ---------- - 20 path : str - 21 path that contains the data files - 22 prefix : str - 23 all files in path that start with prefix are considered as input files. - 24 May be used together postfix to consider only special file endings. - 25 Prefix is ignored, if the keyword 'files' is used. - 26 version : str - 27 version of openQCD, default 2.0 - 28 names : list - 29 list of names that is assigned to the data according according - 30 to the order in the file list. Use careful, if you do not provide file names! - 31 r_start : list - 32 list which contains the first config to be read for each replicum - 33 r_stop : list - 34 list which contains the last config to be read for each replicum - 35 r_step : int - 36 integer that defines a fixed step size between two measurements (in units of configs) - 37 If not given, r_step=1 is assumed. - 38 postfix : str - 39 postfix of the file to read, e.g. '.ms1' for openQCD-files - 40 files : list - 41 list which contains the filenames to be read. No automatic detection of - 42 files performed if given. - 43 print_err : bool - 44 Print additional information that is useful for debugging. - 45 - 46 Returns - 47 ------- - 48 rwms : Obs - 49 Reweighting factors read - 50 """ - 51 known_oqcd_versions = ['1.4', '1.6', '2.0'] - 52 if not (version in known_oqcd_versions): - 53 raise Exception('Unknown openQCD version defined!') - 54 print("Working with openQCD version " + version) - 55 if 'postfix' in kwargs: - 56 postfix = kwargs.get('postfix') - 57 else: - 58 postfix = '' - 59 - 60 if 'files' in kwargs: - 61 known_files = kwargs.get('files') - 62 else: - 63 known_files = [] + 6from ..obs import Obs + 7from ..obs import CObs + 8from ..correlators import Corr + 9from .misc import fit_t0 + 10from .utils import sort_names + 11 + 12 + 13def read_rwms(path, prefix, version='2.0', names=None, **kwargs): + 14 """Read rwms format from given folder structure. Returns a list of length nrw + 15 + 16 Parameters + 17 ---------- + 18 path : str + 19 path that contains the data files + 20 prefix : str + 21 all files in path that start with prefix are considered as input files. + 22 May be used together postfix to consider only special file endings. + 23 Prefix is ignored, if the keyword 'files' is used. + 24 version : str + 25 version of openQCD, default 2.0 + 26 names : list + 27 list of names that is assigned to the data according according + 28 to the order in the file list. Use careful, if you do not provide file names! + 29 r_start : list + 30 list which contains the first config to be read for each replicum + 31 r_stop : list + 32 list which contains the last config to be read for each replicum + 33 r_step : int + 34 integer that defines a fixed step size between two measurements (in units of configs) + 35 If not given, r_step=1 is assumed. + 36 postfix : str + 37 postfix of the file to read, e.g. '.ms1' for openQCD-files + 38 files : list + 39 list which contains the filenames to be read. No automatic detection of + 40 files performed if given. + 41 print_err : bool + 42 Print additional information that is useful for debugging. + 43 + 44 Returns + 45 ------- + 46 rwms : Obs + 47 Reweighting factors read + 48 """ + 49 known_oqcd_versions = ['1.4', '1.6', '2.0'] + 50 if not (version in known_oqcd_versions): + 51 raise Exception('Unknown openQCD version defined!') + 52 print("Working with openQCD version " + version) + 53 if 'postfix' in kwargs: + 54 postfix = kwargs.get('postfix') + 55 else: + 56 postfix = '' + 57 + 58 if 'files' in kwargs: + 59 known_files = kwargs.get('files') + 60 else: + 61 known_files = [] + 62 + 63 ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files) 64 - 65 ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files) + 65 replica = len(ls) 66 - 67 replica = len(ls) - 68 - 69 if 'r_start' in kwargs: - 70 r_start = kwargs.get('r_start') - 71 if len(r_start) != replica: - 72 raise Exception('r_start does not match number of replicas') - 73 r_start = [o if o else None for o in r_start] - 74 else: - 75 r_start = [None] * replica - 76 - 77 if 'r_stop' in kwargs: - 78 r_stop = kwargs.get('r_stop') - 79 if len(r_stop) != replica: - 80 raise Exception('r_stop does not match number of replicas') - 81 else: - 82 r_stop = [None] * replica - 83 - 84 if 'r_step' in kwargs: - 85 r_step = kwargs.get('r_step') - 86 else: - 87 r_step = 1 - 88 - 89 print('Read reweighting factors from', prefix[:-1], ',', - 90 replica, 'replica', end='') - 91 - 92 if names is None: - 93 rep_names = [] - 94 for entry in ls: - 95 truncated_entry = entry - 96 suffixes = [".dat", ".rwms", ".ms1"] - 97 for suffix in suffixes: - 98 if truncated_entry.endswith(suffix): - 99 truncated_entry = truncated_entry[0:-len(suffix)] - 100 idx = truncated_entry.index('r') - 101 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) - 102 else: - 103 rep_names = names + 67 if 'r_start' in kwargs: + 68 r_start = kwargs.get('r_start') + 69 if len(r_start) != replica: + 70 raise Exception('r_start does not match number of replicas') + 71 r_start = [o if o else None for o in r_start] + 72 else: + 73 r_start = [None] * replica + 74 + 75 if 'r_stop' in kwargs: + 76 r_stop = kwargs.get('r_stop') + 77 if len(r_stop) != replica: + 78 raise Exception('r_stop does not match number of replicas') + 79 else: + 80 r_stop = [None] * replica + 81 + 82 if 'r_step' in kwargs: + 83 r_step = kwargs.get('r_step') + 84 else: + 85 r_step = 1 + 86 + 87 print('Read reweighting factors from', prefix[:-1], ',', + 88 replica, 'replica', end='') + 89 + 90 if names is None: + 91 rep_names = [] + 92 for entry in ls: + 93 truncated_entry = entry + 94 suffixes = [".dat", ".rwms", ".ms1"] + 95 for suffix in suffixes: + 96 if truncated_entry.endswith(suffix): + 97 truncated_entry = truncated_entry[0:-len(suffix)] + 98 idx = truncated_entry.index('r') + 99 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) + 100 else: + 101 rep_names = names + 102 + 103 rep_names = sort_names(rep_names) 104 - 105 rep_names = sort_names(rep_names) - 106 - 107 print_err = 0 - 108 if 'print_err' in kwargs: - 109 print_err = 1 - 110 print() + 105 print_err = 0 + 106 if 'print_err' in kwargs: + 107 print_err = 1 + 108 print() + 109 + 110 deltas = [] 111 - 112 deltas = [] - 113 - 114 configlist = [] - 115 r_start_index = [] - 116 r_stop_index = [] - 117 - 118 for rep in range(replica): - 119 tmp_array = [] - 120 with open(path + '/' + ls[rep], 'rb') as fp: - 121 - 122 t = fp.read(4) # number of reweighting factors - 123 if rep == 0: - 124 nrw = struct.unpack('i', t)[0] - 125 if version == '2.0': - 126 nrw = int(nrw / 2) - 127 for k in range(nrw): - 128 deltas.append([]) - 129 else: - 130 if ((nrw != struct.unpack('i', t)[0] and (not version == '2.0')) or (nrw != struct.unpack('i', t)[0] / 2 and version == '2.0')): - 131 raise Exception('Error: different number of reweighting factors for replicum', rep) - 132 - 133 for k in range(nrw): - 134 tmp_array.append([]) - 135 - 136 # This block is necessary for openQCD1.6 and openQCD2.0 ms1 files - 137 nfct = [] - 138 if version in ['1.6', '2.0']: - 139 for i in range(nrw): - 140 t = fp.read(4) - 141 nfct.append(struct.unpack('i', t)[0]) - 142 else: - 143 for i in range(nrw): - 144 nfct.append(1) - 145 - 146 nsrc = [] - 147 for i in range(nrw): - 148 t = fp.read(4) - 149 nsrc.append(struct.unpack('i', t)[0]) - 150 if version == '2.0': - 151 if not struct.unpack('i', fp.read(4))[0] == 0: - 152 raise Exception("You are using the input for openQCD version 2.0, this is not correct.") - 153 - 154 configlist.append([]) - 155 while True: - 156 t = fp.read(4) - 157 if len(t) < 4: - 158 break - 159 config_no = struct.unpack('i', t)[0] - 160 configlist[-1].append(config_no) - 161 for i in range(nrw): - 162 if (version == '2.0'): - 163 tmpd = _read_array_openQCD2(fp) - 164 tmpd = _read_array_openQCD2(fp) - 165 tmp_rw = tmpd['arr'] - 166 tmp_nfct = 1.0 - 167 for j in range(tmpd['n'][0]): - 168 tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw[j]))) - 169 if print_err: - 170 print(config_no, i, j, - 171 np.mean(np.exp(-np.asarray(tmp_rw[j]))), - 172 np.std(np.exp(-np.asarray(tmp_rw[j])))) - 173 print('Sources:', - 174 np.exp(-np.asarray(tmp_rw[j]))) - 175 print('Partial factor:', tmp_nfct) - 176 elif version == '1.6' or version == '1.4': - 177 tmp_nfct = 1.0 - 178 for j in range(nfct[i]): - 179 t = fp.read(8 * nsrc[i]) - 180 t = fp.read(8 * nsrc[i]) - 181 tmp_rw = struct.unpack('d' * nsrc[i], t) - 182 tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw))) - 183 if print_err: - 184 print(config_no, i, j, - 185 np.mean(np.exp(-np.asarray(tmp_rw))), - 186 np.std(np.exp(-np.asarray(tmp_rw)))) - 187 print('Sources:', np.exp(-np.asarray(tmp_rw))) - 188 print('Partial factor:', tmp_nfct) - 189 tmp_array[i].append(tmp_nfct) - 190 - 191 diffmeas = configlist[-1][-1] - configlist[-1][-2] - 192 configlist[-1] = [item // diffmeas for item in configlist[-1]] - 193 if configlist[-1][0] > 1 and diffmeas > 1: - 194 warnings.warn('Assume thermalization and that the first measurement belongs to the first config.') - 195 offset = configlist[-1][0] - 1 - 196 configlist[-1] = [item - offset for item in configlist[-1]] - 197 - 198 if r_start[rep] is None: - 199 r_start_index.append(0) - 200 else: - 201 try: - 202 r_start_index.append(configlist[-1].index(r_start[rep])) - 203 except ValueError: - 204 raise Exception('Config %d not in file with range [%d, %d]' % ( - 205 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None - 206 - 207 if r_stop[rep] is None: - 208 r_stop_index.append(len(configlist[-1]) - 1) - 209 else: - 210 try: - 211 r_stop_index.append(configlist[-1].index(r_stop[rep])) - 212 except ValueError: - 213 raise Exception('Config %d not in file with range [%d, %d]' % ( - 214 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None - 215 - 216 for k in range(nrw): - 217 deltas[k].append(tmp_array[k][r_start_index[rep]:r_stop_index[rep] + 1][::r_step]) - 218 - 219 if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]): - 220 raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist]) - 221 stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist] - 222 if np.any([step != 1 for step in stepsizes]): - 223 warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning) - 224 - 225 print(',', nrw, 'reweighting factors with', nsrc, 'sources') - 226 result = [] - 227 idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)] - 228 - 229 for t in range(nrw): - 230 result.append(Obs(deltas[t], rep_names, idl=idl)) - 231 return result - 232 - 233 - 234def extract_t0(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, postfix='ms', **kwargs): - 235 """Extract t0 from given .ms.dat files. Returns t0 as Obs. - 236 - 237 It is assumed that all boundary effects have - 238 sufficiently decayed at x0=xmin. - 239 The data around the zero crossing of t^2<E> - 0.3 - 240 is fitted with a linear function - 241 from which the exact root is extracted. - 242 - 243 It is assumed that one measurement is performed for each config. - 244 If this is not the case, the resulting idl, as well as the handling - 245 of r_start, r_stop and r_step is wrong and the user has to correct - 246 this in the resulting observable. - 247 - 248 Parameters - 249 ---------- - 250 path : str - 251 Path to .ms.dat files - 252 prefix : str - 253 Ensemble prefix - 254 dtr_read : int - 255 Determines how many trajectories should be skipped - 256 when reading the ms.dat files. - 257 Corresponds to dtr_cnfg / dtr_ms in the openQCD input file. - 258 xmin : int - 259 First timeslice where the boundary - 260 effects have sufficiently decayed. - 261 spatial_extent : int - 262 spatial extent of the lattice, required for normalization. - 263 fit_range : int - 264 Number of data points left and right of the zero - 265 crossing to be included in the linear fit. (Default: 5) - 266 postfix : str - 267 Postfix of measurement file (Default: ms) - 268 r_start : list - 269 list which contains the first config to be read for each replicum. - 270 r_stop : list - 271 list which contains the last config to be read for each replicum. - 272 r_step : int - 273 integer that defines a fixed step size between two measurements (in units of configs) - 274 If not given, r_step=1 is assumed. - 275 plaquette : bool - 276 If true extract the plaquette estimate of t0 instead. - 277 names : list - 278 list of names that is assigned to the data according according - 279 to the order in the file list. Use careful, if you do not provide file names! - 280 files : list - 281 list which contains the filenames to be read. No automatic detection of - 282 files performed if given. - 283 plot_fit : bool - 284 If true, the fit for the extraction of t0 is shown together with the data. - 285 assume_thermalization : bool - 286 If True: If the first record divided by the distance between two measurements is larger than - 287 1, it is assumed that this is due to thermalization and the first measurement belongs - 288 to the first config (default). - 289 If False: The config numbers are assumed to be traj_number // difference - 290 - 291 Returns - 292 ------- - 293 t0 : Obs - 294 Extracted t0 - 295 """ - 296 - 297 if 'files' in kwargs: - 298 known_files = kwargs.get('files') - 299 else: - 300 known_files = [] + 112 configlist = [] + 113 r_start_index = [] + 114 r_stop_index = [] + 115 + 116 for rep in range(replica): + 117 tmp_array = [] + 118 with open(path + '/' + ls[rep], 'rb') as fp: + 119 + 120 t = fp.read(4) # number of reweighting factors + 121 if rep == 0: + 122 nrw = struct.unpack('i', t)[0] + 123 if version == '2.0': + 124 nrw = int(nrw / 2) + 125 for k in range(nrw): + 126 deltas.append([]) + 127 else: + 128 if ((nrw != struct.unpack('i', t)[0] and (not version == '2.0')) or (nrw != struct.unpack('i', t)[0] / 2 and version == '2.0')): + 129 raise Exception('Error: different number of reweighting factors for replicum', rep) + 130 + 131 for k in range(nrw): + 132 tmp_array.append([]) + 133 + 134 # This block is necessary for openQCD1.6 and openQCD2.0 ms1 files + 135 nfct = [] + 136 if version in ['1.6', '2.0']: + 137 for i in range(nrw): + 138 t = fp.read(4) + 139 nfct.append(struct.unpack('i', t)[0]) + 140 else: + 141 for i in range(nrw): + 142 nfct.append(1) + 143 + 144 nsrc = [] + 145 for i in range(nrw): + 146 t = fp.read(4) + 147 nsrc.append(struct.unpack('i', t)[0]) + 148 if version == '2.0': + 149 if not struct.unpack('i', fp.read(4))[0] == 0: + 150 raise Exception("You are using the input for openQCD version 2.0, this is not correct.") + 151 + 152 configlist.append([]) + 153 while True: + 154 t = fp.read(4) + 155 if len(t) < 4: + 156 break + 157 config_no = struct.unpack('i', t)[0] + 158 configlist[-1].append(config_no) + 159 for i in range(nrw): + 160 if (version == '2.0'): + 161 tmpd = _read_array_openQCD2(fp) + 162 tmpd = _read_array_openQCD2(fp) + 163 tmp_rw = tmpd['arr'] + 164 tmp_nfct = 1.0 + 165 for j in range(tmpd['n'][0]): + 166 tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw[j]))) + 167 if print_err: + 168 print(config_no, i, j, + 169 np.mean(np.exp(-np.asarray(tmp_rw[j]))), + 170 np.std(np.exp(-np.asarray(tmp_rw[j])))) + 171 print('Sources:', + 172 np.exp(-np.asarray(tmp_rw[j]))) + 173 print('Partial factor:', tmp_nfct) + 174 elif version == '1.6' or version == '1.4': + 175 tmp_nfct = 1.0 + 176 for j in range(nfct[i]): + 177 t = fp.read(8 * nsrc[i]) + 178 t = fp.read(8 * nsrc[i]) + 179 tmp_rw = struct.unpack('d' * nsrc[i], t) + 180 tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw))) + 181 if print_err: + 182 print(config_no, i, j, + 183 np.mean(np.exp(-np.asarray(tmp_rw))), + 184 np.std(np.exp(-np.asarray(tmp_rw)))) + 185 print('Sources:', np.exp(-np.asarray(tmp_rw))) + 186 print('Partial factor:', tmp_nfct) + 187 tmp_array[i].append(tmp_nfct) + 188 + 189 diffmeas = configlist[-1][-1] - configlist[-1][-2] + 190 configlist[-1] = [item // diffmeas for item in configlist[-1]] + 191 if configlist[-1][0] > 1 and diffmeas > 1: + 192 warnings.warn('Assume thermalization and that the first measurement belongs to the first config.') + 193 offset = configlist[-1][0] - 1 + 194 configlist[-1] = [item - offset for item in configlist[-1]] + 195 + 196 if r_start[rep] is None: + 197 r_start_index.append(0) + 198 else: + 199 try: + 200 r_start_index.append(configlist[-1].index(r_start[rep])) + 201 except ValueError: + 202 raise Exception('Config %d not in file with range [%d, %d]' % ( + 203 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None + 204 + 205 if r_stop[rep] is None: + 206 r_stop_index.append(len(configlist[-1]) - 1) + 207 else: + 208 try: + 209 r_stop_index.append(configlist[-1].index(r_stop[rep])) + 210 except ValueError: + 211 raise Exception('Config %d not in file with range [%d, %d]' % ( + 212 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None + 213 + 214 for k in range(nrw): + 215 deltas[k].append(tmp_array[k][r_start_index[rep]:r_stop_index[rep] + 1][::r_step]) + 216 + 217 if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]): + 218 raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist]) + 219 stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist] + 220 if np.any([step != 1 for step in stepsizes]): + 221 warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning) + 222 + 223 print(',', nrw, 'reweighting factors with', nsrc, 'sources') + 224 result = [] + 225 idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)] + 226 + 227 for t in range(nrw): + 228 result.append(Obs(deltas[t], rep_names, idl=idl)) + 229 return result + 230 + 231 + 232def extract_t0(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, postfix='ms', **kwargs): + 233 """Extract t0 from given .ms.dat files. Returns t0 as Obs. + 234 + 235 It is assumed that all boundary effects have + 236 sufficiently decayed at x0=xmin. + 237 The data around the zero crossing of t^2<E> - 0.3 + 238 is fitted with a linear function + 239 from which the exact root is extracted. + 240 + 241 It is assumed that one measurement is performed for each config. + 242 If this is not the case, the resulting idl, as well as the handling + 243 of r_start, r_stop and r_step is wrong and the user has to correct + 244 this in the resulting observable. + 245 + 246 Parameters + 247 ---------- + 248 path : str + 249 Path to .ms.dat files + 250 prefix : str + 251 Ensemble prefix + 252 dtr_read : int + 253 Determines how many trajectories should be skipped + 254 when reading the ms.dat files. + 255 Corresponds to dtr_cnfg / dtr_ms in the openQCD input file. + 256 xmin : int + 257 First timeslice where the boundary + 258 effects have sufficiently decayed. + 259 spatial_extent : int + 260 spatial extent of the lattice, required for normalization. + 261 fit_range : int + 262 Number of data points left and right of the zero + 263 crossing to be included in the linear fit. (Default: 5) + 264 postfix : str + 265 Postfix of measurement file (Default: ms) + 266 r_start : list + 267 list which contains the first config to be read for each replicum. + 268 r_stop : list + 269 list which contains the last config to be read for each replicum. + 270 r_step : int + 271 integer that defines a fixed step size between two measurements (in units of configs) + 272 If not given, r_step=1 is assumed. + 273 plaquette : bool + 274 If true extract the plaquette estimate of t0 instead. + 275 names : list + 276 list of names that is assigned to the data according according + 277 to the order in the file list. Use careful, if you do not provide file names! + 278 files : list + 279 list which contains the filenames to be read. No automatic detection of + 280 files performed if given. + 281 plot_fit : bool + 282 If true, the fit for the extraction of t0 is shown together with the data. + 283 assume_thermalization : bool + 284 If True: If the first record divided by the distance between two measurements is larger than + 285 1, it is assumed that this is due to thermalization and the first measurement belongs + 286 to the first config (default). + 287 If False: The config numbers are assumed to be traj_number // difference + 288 + 289 Returns + 290 ------- + 291 t0 : Obs + 292 Extracted t0 + 293 """ + 294 + 295 if 'files' in kwargs: + 296 known_files = kwargs.get('files') + 297 else: + 298 known_files = [] + 299 + 300 ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files) 301 - 302 ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files) + 302 replica = len(ls) 303 - 304 replica = len(ls) - 305 - 306 if 'r_start' in kwargs: - 307 r_start = kwargs.get('r_start') - 308 if len(r_start) != replica: - 309 raise Exception('r_start does not match number of replicas') - 310 r_start = [o if o else None for o in r_start] - 311 else: - 312 r_start = [None] * replica - 313 - 314 if 'r_stop' in kwargs: - 315 r_stop = kwargs.get('r_stop') - 316 if len(r_stop) != replica: - 317 raise Exception('r_stop does not match number of replicas') - 318 else: - 319 r_stop = [None] * replica - 320 - 321 if 'r_step' in kwargs: - 322 r_step = kwargs.get('r_step') - 323 else: - 324 r_step = 1 + 304 if 'r_start' in kwargs: + 305 r_start = kwargs.get('r_start') + 306 if len(r_start) != replica: + 307 raise Exception('r_start does not match number of replicas') + 308 r_start = [o if o else None for o in r_start] + 309 else: + 310 r_start = [None] * replica + 311 + 312 if 'r_stop' in kwargs: + 313 r_stop = kwargs.get('r_stop') + 314 if len(r_stop) != replica: + 315 raise Exception('r_stop does not match number of replicas') + 316 else: + 317 r_stop = [None] * replica + 318 + 319 if 'r_step' in kwargs: + 320 r_step = kwargs.get('r_step') + 321 else: + 322 r_step = 1 + 323 + 324 print('Extract t0 from', prefix, ',', replica, 'replica') 325 - 326 print('Extract t0 from', prefix, ',', replica, 'replica') - 327 - 328 if 'names' in kwargs: - 329 rep_names = kwargs.get('names') - 330 else: - 331 rep_names = [] - 332 for entry in ls: - 333 truncated_entry = entry.split('.')[0] - 334 idx = truncated_entry.index('r') - 335 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) + 326 if 'names' in kwargs: + 327 rep_names = kwargs.get('names') + 328 else: + 329 rep_names = [] + 330 for entry in ls: + 331 truncated_entry = entry.split('.')[0] + 332 idx = truncated_entry.index('r') + 333 rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:]) + 334 + 335 Ysum = [] 336 - 337 Ysum = [] - 338 - 339 configlist = [] - 340 r_start_index = [] - 341 r_stop_index = [] + 337 configlist = [] + 338 r_start_index = [] + 339 r_stop_index = [] + 340 + 341 for rep in range(replica): 342 - 343 for rep in range(replica): - 344 - 345 with open(path + '/' + ls[rep], 'rb') as fp: - 346 t = fp.read(12) - 347 header = struct.unpack('iii', t) - 348 if rep == 0: - 349 dn = header[0] - 350 nn = header[1] - 351 tmax = header[2] - 352 elif dn != header[0] or nn != header[1] or tmax != header[2]: - 353 raise Exception('Replica parameters do not match.') - 354 - 355 t = fp.read(8) - 356 if rep == 0: - 357 eps = struct.unpack('d', t)[0] - 358 print('Step size:', eps, ', Maximal t value:', dn * (nn) * eps) - 359 elif eps != struct.unpack('d', t)[0]: - 360 raise Exception('Values for eps do not match among replica.') + 343 with open(path + '/' + ls[rep], 'rb') as fp: + 344 t = fp.read(12) + 345 header = struct.unpack('iii', t) + 346 if rep == 0: + 347 dn = header[0] + 348 nn = header[1] + 349 tmax = header[2] + 350 elif dn != header[0] or nn != header[1] or tmax != header[2]: + 351 raise Exception('Replica parameters do not match.') + 352 + 353 t = fp.read(8) + 354 if rep == 0: + 355 eps = struct.unpack('d', t)[0] + 356 print('Step size:', eps, ', Maximal t value:', dn * (nn) * eps) + 357 elif eps != struct.unpack('d', t)[0]: + 358 raise Exception('Values for eps do not match among replica.') + 359 + 360 Ysl = [] 361 - 362 Ysl = [] - 363 - 364 configlist.append([]) - 365 while True: - 366 t = fp.read(4) - 367 if (len(t) < 4): - 368 break - 369 nc = struct.unpack('i', t)[0] - 370 configlist[-1].append(nc) - 371 - 372 t = fp.read(8 * tmax * (nn + 1)) - 373 if kwargs.get('plaquette'): - 374 if nc % dtr_read == 0: - 375 Ysl.append(struct.unpack('d' * tmax * (nn + 1), t)) - 376 t = fp.read(8 * tmax * (nn + 1)) - 377 if not kwargs.get('plaquette'): - 378 if nc % dtr_read == 0: - 379 Ysl.append(struct.unpack('d' * tmax * (nn + 1), t)) - 380 t = fp.read(8 * tmax * (nn + 1)) - 381 - 382 Ysum.append([]) - 383 for i, item in enumerate(Ysl): - 384 Ysum[-1].append([np.mean(item[current + xmin: - 385 current + tmax - xmin]) - 386 for current in range(0, len(item), tmax)]) - 387 - 388 diffmeas = configlist[-1][-1] - configlist[-1][-2] - 389 configlist[-1] = [item // diffmeas for item in configlist[-1]] - 390 if kwargs.get('assume_thermalization', True) and configlist[-1][0] > 1: - 391 warnings.warn('Assume thermalization and that the first measurement belongs to the first config.') - 392 offset = configlist[-1][0] - 1 - 393 configlist[-1] = [item - offset for item in configlist[-1]] - 394 - 395 if r_start[rep] is None: - 396 r_start_index.append(0) - 397 else: - 398 try: - 399 r_start_index.append(configlist[-1].index(r_start[rep])) - 400 except ValueError: - 401 raise Exception('Config %d not in file with range [%d, %d]' % ( - 402 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None - 403 - 404 if r_stop[rep] is None: - 405 r_stop_index.append(len(configlist[-1]) - 1) - 406 else: - 407 try: - 408 r_stop_index.append(configlist[-1].index(r_stop[rep])) - 409 except ValueError: - 410 raise Exception('Config %d not in file with range [%d, %d]' % ( - 411 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None - 412 - 413 if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]): - 414 raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist]) - 415 stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist] - 416 if np.any([step != 1 for step in stepsizes]): - 417 warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning) - 418 - 419 idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)] - 420 t2E_dict = {} - 421 for n in range(nn + 1): - 422 samples = [] - 423 for nrep, rep in enumerate(Ysum): - 424 samples.append([]) - 425 for cnfg in rep: - 426 samples[-1].append(cnfg[n]) - 427 samples[-1] = samples[-1][r_start_index[nrep]:r_stop_index[nrep] + 1][::r_step] - 428 new_obs = Obs(samples, rep_names, idl=idl) - 429 t2E_dict[n * dn * eps] = (n * dn * eps) ** 2 * new_obs / (spatial_extent ** 3) - 0.3 + 362 configlist.append([]) + 363 while True: + 364 t = fp.read(4) + 365 if (len(t) < 4): + 366 break + 367 nc = struct.unpack('i', t)[0] + 368 configlist[-1].append(nc) + 369 + 370 t = fp.read(8 * tmax * (nn + 1)) + 371 if kwargs.get('plaquette'): + 372 if nc % dtr_read == 0: + 373 Ysl.append(struct.unpack('d' * tmax * (nn + 1), t)) + 374 t = fp.read(8 * tmax * (nn + 1)) + 375 if not kwargs.get('plaquette'): + 376 if nc % dtr_read == 0: + 377 Ysl.append(struct.unpack('d' * tmax * (nn + 1), t)) + 378 t = fp.read(8 * tmax * (nn + 1)) + 379 + 380 Ysum.append([]) + 381 for i, item in enumerate(Ysl): + 382 Ysum[-1].append([np.mean(item[current + xmin: + 383 current + tmax - xmin]) + 384 for current in range(0, len(item), tmax)]) + 385 + 386 diffmeas = configlist[-1][-1] - configlist[-1][-2] + 387 configlist[-1] = [item // diffmeas for item in configlist[-1]] + 388 if kwargs.get('assume_thermalization', True) and configlist[-1][0] > 1: + 389 warnings.warn('Assume thermalization and that the first measurement belongs to the first config.') + 390 offset = configlist[-1][0] - 1 + 391 configlist[-1] = [item - offset for item in configlist[-1]] + 392 + 393 if r_start[rep] is None: + 394 r_start_index.append(0) + 395 else: + 396 try: + 397 r_start_index.append(configlist[-1].index(r_start[rep])) + 398 except ValueError: + 399 raise Exception('Config %d not in file with range [%d, %d]' % ( + 400 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None + 401 + 402 if r_stop[rep] is None: + 403 r_stop_index.append(len(configlist[-1]) - 1) + 404 else: + 405 try: + 406 r_stop_index.append(configlist[-1].index(r_stop[rep])) + 407 except ValueError: + 408 raise Exception('Config %d not in file with range [%d, %d]' % ( + 409 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None + 410 + 411 if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]): + 412 raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist]) + 413 stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist] + 414 if np.any([step != 1 for step in stepsizes]): + 415 warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning) + 416 + 417 idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)] + 418 t2E_dict = {} + 419 for n in range(nn + 1): + 420 samples = [] + 421 for nrep, rep in enumerate(Ysum): + 422 samples.append([]) + 423 for cnfg in rep: + 424 samples[-1].append(cnfg[n]) + 425 samples[-1] = samples[-1][r_start_index[nrep]:r_stop_index[nrep] + 1][::r_step] + 426 new_obs = Obs(samples, rep_names, idl=idl) + 427 t2E_dict[n * dn * eps] = (n * dn * eps) ** 2 * new_obs / (spatial_extent ** 3) - 0.3 + 428 + 429 return fit_t0(t2E_dict, fit_range, plot_fit=kwargs.get('plot_fit')) 430 - 431 zero_crossing = np.argmax(np.array( - 432 [o.value for o in t2E_dict.values()]) > 0.0) - 433 - 434 x = list(t2E_dict.keys())[zero_crossing - fit_range: - 435 zero_crossing + fit_range] - 436 y = list(t2E_dict.values())[zero_crossing - fit_range: - 437 zero_crossing + fit_range] - 438 [o.gamma_method() for o in y] - 439 - 440 fit_result = fit_lin(x, y) - 441 - 442 if kwargs.get('plot_fit'): - 443 plt.figure() - 444 gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0) - 445 ax0 = plt.subplot(gs[0]) - 446 xmore = list(t2E_dict.keys())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2] - 447 ymore = list(t2E_dict.values())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2] - 448 [o.gamma_method() for o in ymore] - 449 ax0.errorbar(xmore, [yi.value for yi in ymore], yerr=[yi.dvalue for yi in ymore], fmt='x') - 450 xplot = np.linspace(np.min(x), np.max(x)) - 451 yplot = [fit_result[0] + fit_result[1] * xi for xi in xplot] - 452 [yi.gamma_method() for yi in yplot] - 453 ax0.fill_between(xplot, y1=[yi.value - yi.dvalue for yi in yplot], y2=[yi.value + yi.dvalue for yi in yplot]) - 454 retval = (-fit_result[0] / fit_result[1]) - 455 retval.gamma_method() - 456 ylim = ax0.get_ylim() - 457 ax0.fill_betweenx(ylim, x1=retval.value - retval.dvalue, x2=retval.value + retval.dvalue, color='gray', alpha=0.4) - 458 ax0.set_ylim(ylim) - 459 ax0.set_ylabel(r'$t^2 \langle E(t) \rangle - 0.3 $') - 460 xlim = ax0.get_xlim() - 461 - 462 fit_res = [fit_result[0] + fit_result[1] * xi for xi in x] - 463 residuals = (np.asarray([o.value for o in y]) - [o.value for o in fit_res]) / np.asarray([o.dvalue for o in y]) - 464 ax1 = plt.subplot(gs[1]) - 465 ax1.plot(x, residuals, 'ko', ls='none', markersize=5) - 466 ax1.tick_params(direction='out') - 467 ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True) - 468 ax1.axhline(y=0.0, ls='--', color='k') - 469 ax1.fill_between(xlim, -1.0, 1.0, alpha=0.1, facecolor='k') - 470 ax1.set_xlim(xlim) - 471 ax1.set_ylabel('Residuals') - 472 ax1.set_xlabel(r'$t/a^2$') - 473 - 474 plt.draw() - 475 return -fit_result[0] / fit_result[1] + 431 + 432def _parse_array_openQCD2(d, n, size, wa, quadrupel=False): + 433 arr = [] + 434 if d == 2: + 435 for i in range(n[0]): + 436 tmp = wa[i * n[1]:(i + 1) * n[1]] + 437 if quadrupel: + 438 tmp2 = [] + 439 for j in range(0, len(tmp), 2): + 440 tmp2.append(tmp[j]) + 441 arr.append(tmp2) + 442 else: + 443 arr.append(np.asarray(tmp)) + 444 + 445 else: + 446 raise Exception('Only two-dimensional arrays supported!') + 447 + 448 return arr + 449 + 450 + 451def _find_files(path, prefix, postfix, ext, known_files=[]): + 452 found = [] + 453 files = [] + 454 + 455 if postfix != "": + 456 if postfix[-1] != ".": + 457 postfix = postfix + "." + 458 if postfix[0] != ".": + 459 postfix = "." + postfix + 460 + 461 if ext[0] == ".": + 462 ext = ext[1:] + 463 + 464 pattern = prefix + "*" + postfix + ext + 465 + 466 for (dirpath, dirnames, filenames) in os.walk(path + "/"): + 467 found.extend(filenames) + 468 break + 469 + 470 if known_files != []: + 471 for kf in known_files: + 472 if kf not in found: + 473 raise FileNotFoundError("Given file " + kf + " does not exist!") + 474 + 475 return known_files 476 - 477 - 478def _parse_array_openQCD2(d, n, size, wa, quadrupel=False): - 479 arr = [] - 480 if d == 2: - 481 for i in range(n[0]): - 482 tmp = wa[i * n[1]:(i + 1) * n[1]] - 483 if quadrupel: - 484 tmp2 = [] - 485 for j in range(0, len(tmp), 2): - 486 tmp2.append(tmp[j]) - 487 arr.append(tmp2) - 488 else: - 489 arr.append(np.asarray(tmp)) + 477 if not found: + 478 raise FileNotFoundError(f"Error, directory '{path}' not found") + 479 + 480 for f in found: + 481 if fnmatch.fnmatch(f, pattern): + 482 files.append(f) + 483 + 484 if files == []: + 485 raise Exception("No files found after pattern filter!") + 486 + 487 files = sort_names(files) + 488 return files + 489 490 - 491 else: - 492 raise Exception('Only two-dimensional arrays supported!') - 493 - 494 return arr - 495 - 496 - 497def _find_files(path, prefix, postfix, ext, known_files=[]): - 498 found = [] - 499 files = [] - 500 - 501 if postfix != "": - 502 if postfix[-1] != ".": - 503 postfix = postfix + "." - 504 if postfix[0] != ".": - 505 postfix = "." + postfix - 506 - 507 if ext[0] == ".": - 508 ext = ext[1:] + 491def _read_array_openQCD2(fp): + 492 t = fp.read(4) + 493 d = struct.unpack('i', t)[0] + 494 t = fp.read(4 * d) + 495 n = struct.unpack('%di' % (d), t) + 496 t = fp.read(4) + 497 size = struct.unpack('i', t)[0] + 498 if size == 4: + 499 types = 'i' + 500 elif size == 8: + 501 types = 'd' + 502 elif size == 16: + 503 types = 'dd' + 504 else: + 505 raise Exception("Type for size '" + str(size) + "' not known.") + 506 m = n[0] + 507 for i in range(1, d): + 508 m *= n[i] 509 - 510 pattern = prefix + "*" + postfix + ext - 511 - 512 for (dirpath, dirnames, filenames) in os.walk(path + "/"): - 513 found.extend(filenames) - 514 break + 510 t = fp.read(m * size) + 511 tmp = struct.unpack('%d%s' % (m, types), t) + 512 + 513 arr = _parse_array_openQCD2(d, n, size, tmp, quadrupel=True) + 514 return {'d': d, 'n': n, 'size': size, 'arr': arr} 515 - 516 if known_files != []: - 517 for kf in known_files: - 518 if kf not in found: - 519 raise FileNotFoundError("Given file " + kf + " does not exist!") - 520 - 521 return known_files - 522 - 523 if not found: - 524 raise FileNotFoundError(f"Error, directory '{path}' not found") - 525 - 526 for f in found: - 527 if fnmatch.fnmatch(f, pattern): - 528 files.append(f) - 529 - 530 if files == []: - 531 raise Exception("No files found after pattern filter!") - 532 - 533 files = sort_names(files) - 534 return files - 535 - 536 - 537def _read_array_openQCD2(fp): - 538 t = fp.read(4) - 539 d = struct.unpack('i', t)[0] - 540 t = fp.read(4 * d) - 541 n = struct.unpack('%di' % (d), t) - 542 t = fp.read(4) - 543 size = struct.unpack('i', t)[0] - 544 if size == 4: - 545 types = 'i' - 546 elif size == 8: - 547 types = 'd' - 548 elif size == 16: - 549 types = 'dd' - 550 else: - 551 raise Exception("Type for size '" + str(size) + "' not known.") - 552 m = n[0] - 553 for i in range(1, d): - 554 m *= n[i] - 555 - 556 t = fp.read(m * size) - 557 tmp = struct.unpack('%d%s' % (m, types), t) - 558 - 559 arr = _parse_array_openQCD2(d, n, size, tmp, quadrupel=True) - 560 return {'d': d, 'n': n, 'size': size, 'arr': arr} - 561 - 562 - 563def read_qtop(path, prefix, c, dtr_cnfg=1, version="openQCD", **kwargs): - 564 """Read the topologial charge based on openQCD gradient flow measurements. - 565 - 566 Parameters - 567 ---------- - 568 path : str - 569 path of the measurement files - 570 prefix : str - 571 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. - 572 Ignored if file names are passed explicitly via keyword files. - 573 c : double - 574 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. - 575 dtr_cnfg : int - 576 (optional) parameter that specifies the number of measurements - 577 between two configs. - 578 If it is not set, the distance between two measurements - 579 in the file is assumed to be the distance between two configurations. - 580 steps : int - 581 (optional) Distance between two configurations in units of trajectories / - 582 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given - 583 version : str - 584 Either openQCD or sfqcd, depending on the data. - 585 L : int - 586 spatial length of the lattice in L/a. - 587 HAS to be set if version != sfqcd, since openQCD does not provide - 588 this in the header - 589 r_start : list - 590 list which contains the first config to be read for each replicum. - 591 r_stop : list - 592 list which contains the last config to be read for each replicum. - 593 files : list - 594 specify the exact files that need to be read - 595 from path, practical if e.g. only one replicum is needed - 596 postfix : str - 597 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files - 598 names : list - 599 Alternative labeling for replicas/ensembles. - 600 Has to have the appropriate length. - 601 Zeuthen_flow : bool - 602 (optional) If True, the Zeuthen flow is used for Qtop. Only possible - 603 for version=='sfqcd' If False, the Wilson flow is used. - 604 integer_charge : bool - 605 If True, the charge is rounded towards the nearest integer on each config. - 606 - 607 Returns - 608 ------- - 609 result : Obs - 610 Read topological charge - 611 """ - 612 - 613 return _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version=version, obspos=0, **kwargs) - 614 + 516 + 517def read_qtop(path, prefix, c, dtr_cnfg=1, version="openQCD", **kwargs): + 518 """Read the topologial charge based on openQCD gradient flow measurements. + 519 + 520 Parameters + 521 ---------- + 522 path : str + 523 path of the measurement files + 524 prefix : str + 525 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. + 526 Ignored if file names are passed explicitly via keyword files. + 527 c : double + 528 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. + 529 dtr_cnfg : int + 530 (optional) parameter that specifies the number of measurements + 531 between two configs. + 532 If it is not set, the distance between two measurements + 533 in the file is assumed to be the distance between two configurations. + 534 steps : int + 535 (optional) Distance between two configurations in units of trajectories / + 536 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given + 537 version : str + 538 Either openQCD or sfqcd, depending on the data. + 539 L : int + 540 spatial length of the lattice in L/a. + 541 HAS to be set if version != sfqcd, since openQCD does not provide + 542 this in the header + 543 r_start : list + 544 list which contains the first config to be read for each replicum. + 545 r_stop : list + 546 list which contains the last config to be read for each replicum. + 547 files : list + 548 specify the exact files that need to be read + 549 from path, practical if e.g. only one replicum is needed + 550 postfix : str + 551 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files + 552 names : list + 553 Alternative labeling for replicas/ensembles. + 554 Has to have the appropriate length. + 555 Zeuthen_flow : bool + 556 (optional) If True, the Zeuthen flow is used for Qtop. Only possible + 557 for version=='sfqcd' If False, the Wilson flow is used. + 558 integer_charge : bool + 559 If True, the charge is rounded towards the nearest integer on each config. + 560 + 561 Returns + 562 ------- + 563 result : Obs + 564 Read topological charge + 565 """ + 566 + 567 return _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version=version, obspos=0, **kwargs) + 568 + 569 + 570def read_gf_coupling(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs): + 571 """Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details. + 572 + 573 Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step. + 574 + 575 Parameters + 576 ---------- + 577 path : str + 578 path of the measurement files + 579 prefix : str + 580 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. + 581 Ignored if file names are passed explicitly via keyword files. + 582 c : double + 583 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. + 584 dtr_cnfg : int + 585 (optional) parameter that specifies the number of measurements + 586 between two configs. + 587 If it is not set, the distance between two measurements + 588 in the file is assumed to be the distance between two configurations. + 589 steps : int + 590 (optional) Distance between two configurations in units of trajectories / + 591 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given + 592 r_start : list + 593 list which contains the first config to be read for each replicum. + 594 r_stop : list + 595 list which contains the last config to be read for each replicum. + 596 files : list + 597 specify the exact files that need to be read + 598 from path, practical if e.g. only one replicum is needed + 599 names : list + 600 Alternative labeling for replicas/ensembles. + 601 Has to have the appropriate length. + 602 postfix : str + 603 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files + 604 Zeuthen_flow : bool + 605 (optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used. + 606 """ + 607 + 608 if c != 0.3: + 609 raise Exception("The required lattice norm is only implemented for c=0.3 at the moment.") + 610 + 611 plaq = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=6, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs) + 612 C2x1 = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=7, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs) + 613 L = plaq.tag["L"] + 614 T = plaq.tag["T"] 615 - 616def read_gf_coupling(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs): - 617 """Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details. + 616 if T != L: + 617 raise Exception("The required lattice norm is only implemented for T=L at the moment.") 618 - 619 Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step. - 620 - 621 Parameters - 622 ---------- - 623 path : str - 624 path of the measurement files - 625 prefix : str - 626 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. - 627 Ignored if file names are passed explicitly via keyword files. - 628 c : double - 629 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. - 630 dtr_cnfg : int - 631 (optional) parameter that specifies the number of measurements - 632 between two configs. - 633 If it is not set, the distance between two measurements - 634 in the file is assumed to be the distance between two configurations. - 635 steps : int - 636 (optional) Distance between two configurations in units of trajectories / - 637 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given - 638 r_start : list - 639 list which contains the first config to be read for each replicum. - 640 r_stop : list - 641 list which contains the last config to be read for each replicum. - 642 files : list - 643 specify the exact files that need to be read - 644 from path, practical if e.g. only one replicum is needed - 645 names : list - 646 Alternative labeling for replicas/ensembles. - 647 Has to have the appropriate length. - 648 postfix : str - 649 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files - 650 Zeuthen_flow : bool - 651 (optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used. - 652 """ - 653 - 654 if c != 0.3: - 655 raise Exception("The required lattice norm is only implemented for c=0.3 at the moment.") - 656 - 657 plaq = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=6, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs) - 658 C2x1 = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=7, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs) - 659 L = plaq.tag["L"] - 660 T = plaq.tag["T"] - 661 - 662 if T != L: - 663 raise Exception("The required lattice norm is only implemented for T=L at the moment.") - 664 - 665 if Zeuthen_flow is not True: - 666 raise Exception("The required lattice norm is only implemented for the Zeuthen flow at the moment.") - 667 - 668 t = (c * L) ** 2 / 8 - 669 - 670 normdict = {4: 0.012341170468270, - 671 6: 0.010162691462430, - 672 8: 0.009031614807931, - 673 10: 0.008744966371393, - 674 12: 0.008650917856809, - 675 14: 8.611154391267955E-03, - 676 16: 0.008591758449508, - 677 20: 0.008575359627103, - 678 24: 0.008569387847540, - 679 28: 8.566803713382559E-03, - 680 32: 0.008565541650006, - 681 40: 8.564480684962046E-03, - 682 48: 8.564098025073460E-03, - 683 64: 8.563853943383087E-03} - 684 - 685 return t * t * (5 / 3 * plaq - 1 / 12 * C2x1) / normdict[L] - 686 - 687 - 688def _read_flow_obs(path, prefix, c, dtr_cnfg=1, version="openQCD", obspos=0, sum_t=True, **kwargs): - 689 """Read a flow observable based on openQCD gradient flow measurements. - 690 - 691 Parameters - 692 ---------- - 693 path : str - 694 path of the measurement files - 695 prefix : str - 696 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. - 697 Ignored if file names are passed explicitly via keyword files. - 698 c : double - 699 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. - 700 dtr_cnfg : int - 701 (optional) parameter that specifies the number of measurements - 702 between two configs. - 703 If it is not set, the distance between two measurements - 704 in the file is assumed to be the distance between two configurations. - 705 steps : int - 706 (optional) Distance between two configurations in units of trajectories / - 707 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given - 708 version : str - 709 Either openQCD or sfqcd, depending on the data. - 710 obspos : int - 711 position of the obeservable in the measurement file. Only relevant for sfqcd files. - 712 sum_t : bool - 713 If true sum over all timeslices, if false only take the value at T/2. - 714 L : int - 715 spatial length of the lattice in L/a. - 716 HAS to be set if version != sfqcd, since openQCD does not provide - 717 this in the header - 718 r_start : list - 719 list which contains the first config to be read for each replicum. - 720 r_stop : list - 721 list which contains the last config to be read for each replicum. - 722 files : list - 723 specify the exact files that need to be read - 724 from path, practical if e.g. only one replicum is needed - 725 names : list - 726 Alternative labeling for replicas/ensembles. - 727 Has to have the appropriate length. - 728 postfix : str - 729 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files - 730 Zeuthen_flow : bool - 731 (optional) If True, the Zeuthen flow is used for Qtop. Only possible - 732 for version=='sfqcd' If False, the Wilson flow is used. - 733 integer_charge : bool - 734 If True, the charge is rounded towards the nearest integer on each config. - 735 - 736 Returns - 737 ------- - 738 result : Obs - 739 flow observable specified - 740 """ - 741 known_versions = ["openQCD", "sfqcd"] - 742 - 743 if version not in known_versions: - 744 raise Exception("Unknown openQCD version.") - 745 if "steps" in kwargs: - 746 steps = kwargs.get("steps") - 747 if version == "sfqcd": - 748 if "L" in kwargs: - 749 supposed_L = kwargs.get("L") - 750 else: - 751 supposed_L = None - 752 postfix = "gfms" - 753 else: - 754 if "L" not in kwargs: - 755 raise Exception("This version of openQCD needs you to provide the spatial length of the lattice as parameter 'L'.") - 756 else: - 757 L = kwargs.get("L") - 758 postfix = "ms" - 759 - 760 if "postfix" in kwargs: - 761 postfix = kwargs.get("postfix") - 762 - 763 if "files" in kwargs: - 764 known_files = kwargs.get("files") - 765 else: - 766 known_files = [] - 767 - 768 files = _find_files(path, prefix, postfix, "dat", known_files=known_files) - 769 - 770 if 'r_start' in kwargs: - 771 r_start = kwargs.get('r_start') - 772 if len(r_start) != len(files): - 773 raise Exception('r_start does not match number of replicas') - 774 r_start = [o if o else None for o in r_start] - 775 else: - 776 r_start = [None] * len(files) - 777 - 778 if 'r_stop' in kwargs: - 779 r_stop = kwargs.get('r_stop') - 780 if len(r_stop) != len(files): - 781 raise Exception('r_stop does not match number of replicas') - 782 else: - 783 r_stop = [None] * len(files) - 784 rep_names = [] - 785 - 786 zeuthen = kwargs.get('Zeuthen_flow', False) - 787 if zeuthen and version not in ['sfqcd']: - 788 raise Exception('Zeuthen flow can only be used for version==sfqcd') - 789 - 790 r_start_index = [] - 791 r_stop_index = [] - 792 deltas = [] - 793 configlist = [] - 794 if not zeuthen: - 795 obspos += 8 - 796 for rep, file in enumerate(files): - 797 with open(path + "/" + file, "rb") as fp: - 798 - 799 Q = [] - 800 traj_list = [] - 801 if version in ['sfqcd']: - 802 t = fp.read(12) - 803 header = struct.unpack('<iii', t) - 804 zthfl = header[0] # Zeuthen flow -> if it's equal to 2 it means that the Zeuthen flow is also 'measured' (apart from the Wilson flow) - 805 ncs = header[1] # number of different values for c in t_flow=1/8 c² L² -> measurements done for ncs c's - 806 tmax = header[2] # lattice T/a - 807 - 808 t = fp.read(12) - 809 Ls = struct.unpack('<iii', t) - 810 if (Ls[0] == Ls[1] and Ls[1] == Ls[2]): - 811 L = Ls[0] - 812 if not (supposed_L == L) and supposed_L: - 813 raise Exception("It seems the length given in the header and by you contradict each other") - 814 else: - 815 raise Exception("Found more than one spatial length in header!") - 816 - 817 t = fp.read(16) - 818 header2 = struct.unpack('<dd', t) - 819 tol = header2[0] - 820 cmax = header2[1] # highest value of c used - 821 - 822 if c > cmax: - 823 raise Exception('Flow has been determined between c=0 and c=%lf with tolerance %lf' % (cmax, tol)) - 824 - 825 if (zthfl == 2): - 826 nfl = 2 # number of flows - 827 else: - 828 nfl = 1 - 829 iobs = 8 * nfl # number of flow observables calculated - 830 - 831 while True: - 832 t = fp.read(4) - 833 if (len(t) < 4): - 834 break - 835 traj_list.append(struct.unpack('i', t)[0]) # trajectory number when measurement was done - 836 - 837 for j in range(ncs + 1): - 838 for i in range(iobs): - 839 t = fp.read(8 * tmax) - 840 if (i == obspos): # determines the flow observable -> i=0 <-> Zeuthen flow - 841 Q.append(struct.unpack('d' * tmax, t)) + 619 if Zeuthen_flow is not True: + 620 raise Exception("The required lattice norm is only implemented for the Zeuthen flow at the moment.") + 621 + 622 t = (c * L) ** 2 / 8 + 623 + 624 normdict = {4: 0.012341170468270, + 625 6: 0.010162691462430, + 626 8: 0.009031614807931, + 627 10: 0.008744966371393, + 628 12: 0.008650917856809, + 629 14: 8.611154391267955E-03, + 630 16: 0.008591758449508, + 631 20: 0.008575359627103, + 632 24: 0.008569387847540, + 633 28: 8.566803713382559E-03, + 634 32: 0.008565541650006, + 635 40: 8.564480684962046E-03, + 636 48: 8.564098025073460E-03, + 637 64: 8.563853943383087E-03} + 638 + 639 return t * t * (5 / 3 * plaq - 1 / 12 * C2x1) / normdict[L] + 640 + 641 + 642def _read_flow_obs(path, prefix, c, dtr_cnfg=1, version="openQCD", obspos=0, sum_t=True, **kwargs): + 643 """Read a flow observable based on openQCD gradient flow measurements. + 644 + 645 Parameters + 646 ---------- + 647 path : str + 648 path of the measurement files + 649 prefix : str + 650 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat. + 651 Ignored if file names are passed explicitly via keyword files. + 652 c : double + 653 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L. + 654 dtr_cnfg : int + 655 (optional) parameter that specifies the number of measurements + 656 between two configs. + 657 If it is not set, the distance between two measurements + 658 in the file is assumed to be the distance between two configurations. + 659 steps : int + 660 (optional) Distance between two configurations in units of trajectories / + 661 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given + 662 version : str + 663 Either openQCD or sfqcd, depending on the data. + 664 obspos : int + 665 position of the obeservable in the measurement file. Only relevant for sfqcd files. + 666 sum_t : bool + 667 If true sum over all timeslices, if false only take the value at T/2. + 668 L : int + 669 spatial length of the lattice in L/a. + 670 HAS to be set if version != sfqcd, since openQCD does not provide + 671 this in the header + 672 r_start : list + 673 list which contains the first config to be read for each replicum. + 674 r_stop : list + 675 list which contains the last config to be read for each replicum. + 676 files : list + 677 specify the exact files that need to be read + 678 from path, practical if e.g. only one replicum is needed + 679 names : list + 680 Alternative labeling for replicas/ensembles. + 681 Has to have the appropriate length. + 682 postfix : str + 683 postfix of the file to read, e.g. '.gfms.dat' for openQCD-files + 684 Zeuthen_flow : bool + 685 (optional) If True, the Zeuthen flow is used for Qtop. Only possible + 686 for version=='sfqcd' If False, the Wilson flow is used. + 687 integer_charge : bool + 688 If True, the charge is rounded towards the nearest integer on each config. + 689 + 690 Returns + 691 ------- + 692 result : Obs + 693 flow observable specified + 694 """ + 695 known_versions = ["openQCD", "sfqcd"] + 696 + 697 if version not in known_versions: + 698 raise Exception("Unknown openQCD version.") + 699 if "steps" in kwargs: + 700 steps = kwargs.get("steps") + 701 if version == "sfqcd": + 702 if "L" in kwargs: + 703 supposed_L = kwargs.get("L") + 704 else: + 705 supposed_L = None + 706 postfix = "gfms" + 707 else: + 708 if "L" not in kwargs: + 709 raise Exception("This version of openQCD needs you to provide the spatial length of the lattice as parameter 'L'.") + 710 else: + 711 L = kwargs.get("L") + 712 postfix = "ms" + 713 + 714 if "postfix" in kwargs: + 715 postfix = kwargs.get("postfix") + 716 + 717 if "files" in kwargs: + 718 known_files = kwargs.get("files") + 719 else: + 720 known_files = [] + 721 + 722 files = _find_files(path, prefix, postfix, "dat", known_files=known_files) + 723 + 724 if 'r_start' in kwargs: + 725 r_start = kwargs.get('r_start') + 726 if len(r_start) != len(files): + 727 raise Exception('r_start does not match number of replicas') + 728 r_start = [o if o else None for o in r_start] + 729 else: + 730 r_start = [None] * len(files) + 731 + 732 if 'r_stop' in kwargs: + 733 r_stop = kwargs.get('r_stop') + 734 if len(r_stop) != len(files): + 735 raise Exception('r_stop does not match number of replicas') + 736 else: + 737 r_stop = [None] * len(files) + 738 rep_names = [] + 739 + 740 zeuthen = kwargs.get('Zeuthen_flow', False) + 741 if zeuthen and version not in ['sfqcd']: + 742 raise Exception('Zeuthen flow can only be used for version==sfqcd') + 743 + 744 r_start_index = [] + 745 r_stop_index = [] + 746 deltas = [] + 747 configlist = [] + 748 if not zeuthen: + 749 obspos += 8 + 750 for rep, file in enumerate(files): + 751 with open(path + "/" + file, "rb") as fp: + 752 + 753 Q = [] + 754 traj_list = [] + 755 if version in ['sfqcd']: + 756 t = fp.read(12) + 757 header = struct.unpack('<iii', t) + 758 zthfl = header[0] # Zeuthen flow -> if it's equal to 2 it means that the Zeuthen flow is also 'measured' (apart from the Wilson flow) + 759 ncs = header[1] # number of different values for c in t_flow=1/8 c² L² -> measurements done for ncs c's + 760 tmax = header[2] # lattice T/a + 761 + 762 t = fp.read(12) + 763 Ls = struct.unpack('<iii', t) + 764 if (Ls[0] == Ls[1] and Ls[1] == Ls[2]): + 765 L = Ls[0] + 766 if not (supposed_L == L) and supposed_L: + 767 raise Exception("It seems the length given in the header and by you contradict each other") + 768 else: + 769 raise Exception("Found more than one spatial length in header!") + 770 + 771 t = fp.read(16) + 772 header2 = struct.unpack('<dd', t) + 773 tol = header2[0] + 774 cmax = header2[1] # highest value of c used + 775 + 776 if c > cmax: + 777 raise Exception('Flow has been determined between c=0 and c=%lf with tolerance %lf' % (cmax, tol)) + 778 + 779 if (zthfl == 2): + 780 nfl = 2 # number of flows + 781 else: + 782 nfl = 1 + 783 iobs = 8 * nfl # number of flow observables calculated + 784 + 785 while True: + 786 t = fp.read(4) + 787 if (len(t) < 4): + 788 break + 789 traj_list.append(struct.unpack('i', t)[0]) # trajectory number when measurement was done + 790 + 791 for j in range(ncs + 1): + 792 for i in range(iobs): + 793 t = fp.read(8 * tmax) + 794 if (i == obspos): # determines the flow observable -> i=0 <-> Zeuthen flow + 795 Q.append(struct.unpack('d' * tmax, t)) + 796 + 797 else: + 798 t = fp.read(12) + 799 header = struct.unpack('<iii', t) + 800 # step size in integration steps "dnms" + 801 dn = header[0] + 802 # number of measurements, so "ntot"/dn + 803 nn = header[1] + 804 # lattice T/a + 805 tmax = header[2] + 806 + 807 t = fp.read(8) + 808 eps = struct.unpack('d', t)[0] + 809 + 810 while True: + 811 t = fp.read(4) + 812 if (len(t) < 4): + 813 break + 814 traj_list.append(struct.unpack('i', t)[0]) + 815 # Wsl + 816 t = fp.read(8 * tmax * (nn + 1)) + 817 # Ysl + 818 t = fp.read(8 * tmax * (nn + 1)) + 819 # Qsl, which is asked for in this method + 820 t = fp.read(8 * tmax * (nn + 1)) + 821 # unpack the array of Qtops, + 822 # on each timeslice t=0,...,tmax-1 and the + 823 # measurement number in = 0...nn (see README.qcd1) + 824 tmpd = struct.unpack('d' * tmax * (nn + 1), t) + 825 Q.append(tmpd) + 826 + 827 if len(np.unique(np.diff(traj_list))) != 1: + 828 raise Exception("Irregularities in stepsize found") + 829 else: + 830 if 'steps' in kwargs: + 831 if steps != traj_list[1] - traj_list[0]: + 832 raise Exception("steps and the found stepsize are not the same") + 833 else: + 834 steps = traj_list[1] - traj_list[0] + 835 + 836 configlist.append([tr // steps // dtr_cnfg for tr in traj_list]) + 837 if configlist[-1][0] > 1: + 838 offset = configlist[-1][0] - 1 + 839 warnings.warn('Assume thermalization and that the first measurement belongs to the first config. Offset = %d configs (%d trajectories / cycles)' % ( + 840 offset, offset * steps)) + 841 configlist[-1] = [item - offset for item in configlist[-1]] 842 - 843 else: - 844 t = fp.read(12) - 845 header = struct.unpack('<iii', t) - 846 # step size in integration steps "dnms" - 847 dn = header[0] - 848 # number of measurements, so "ntot"/dn - 849 nn = header[1] - 850 # lattice T/a - 851 tmax = header[2] - 852 - 853 t = fp.read(8) - 854 eps = struct.unpack('d', t)[0] - 855 - 856 while True: - 857 t = fp.read(4) - 858 if (len(t) < 4): - 859 break - 860 traj_list.append(struct.unpack('i', t)[0]) - 861 # Wsl - 862 t = fp.read(8 * tmax * (nn + 1)) - 863 # Ysl - 864 t = fp.read(8 * tmax * (nn + 1)) - 865 # Qsl, which is asked for in this method - 866 t = fp.read(8 * tmax * (nn + 1)) - 867 # unpack the array of Qtops, - 868 # on each timeslice t=0,...,tmax-1 and the - 869 # measurement number in = 0...nn (see README.qcd1) - 870 tmpd = struct.unpack('d' * tmax * (nn + 1), t) - 871 Q.append(tmpd) - 872 - 873 if len(np.unique(np.diff(traj_list))) != 1: - 874 raise Exception("Irregularities in stepsize found") - 875 else: - 876 if 'steps' in kwargs: - 877 if steps != traj_list[1] - traj_list[0]: - 878 raise Exception("steps and the found stepsize are not the same") - 879 else: - 880 steps = traj_list[1] - traj_list[0] - 881 - 882 configlist.append([tr // steps // dtr_cnfg for tr in traj_list]) - 883 if configlist[-1][0] > 1: - 884 offset = configlist[-1][0] - 1 - 885 warnings.warn('Assume thermalization and that the first measurement belongs to the first config. Offset = %d configs (%d trajectories / cycles)' % ( - 886 offset, offset * steps)) - 887 configlist[-1] = [item - offset for item in configlist[-1]] - 888 - 889 if r_start[rep] is None: - 890 r_start_index.append(0) - 891 else: - 892 try: - 893 r_start_index.append(configlist[-1].index(r_start[rep])) - 894 except ValueError: - 895 raise Exception('Config %d not in file with range [%d, %d]' % ( - 896 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None - 897 - 898 if r_stop[rep] is None: - 899 r_stop_index.append(len(configlist[-1]) - 1) - 900 else: - 901 try: - 902 r_stop_index.append(configlist[-1].index(r_stop[rep])) - 903 except ValueError: - 904 raise Exception('Config %d not in file with range [%d, %d]' % ( - 905 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None - 906 - 907 if version in ['sfqcd']: - 908 cstepsize = cmax / ncs - 909 index_aim = round(c / cstepsize) - 910 else: - 911 t_aim = (c * L) ** 2 / 8 - 912 index_aim = round(t_aim / eps / dn) + 843 if r_start[rep] is None: + 844 r_start_index.append(0) + 845 else: + 846 try: + 847 r_start_index.append(configlist[-1].index(r_start[rep])) + 848 except ValueError: + 849 raise Exception('Config %d not in file with range [%d, %d]' % ( + 850 r_start[rep], configlist[-1][0], configlist[-1][-1])) from None + 851 + 852 if r_stop[rep] is None: + 853 r_stop_index.append(len(configlist[-1]) - 1) + 854 else: + 855 try: + 856 r_stop_index.append(configlist[-1].index(r_stop[rep])) + 857 except ValueError: + 858 raise Exception('Config %d not in file with range [%d, %d]' % ( + 859 r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None + 860 + 861 if version in ['sfqcd']: + 862 cstepsize = cmax / ncs + 863 index_aim = round(c / cstepsize) + 864 else: + 865 t_aim = (c * L) ** 2 / 8 + 866 index_aim = round(t_aim / eps / dn) + 867 + 868 Q_sum = [] + 869 for i, item in enumerate(Q): + 870 if sum_t is True: + 871 Q_sum.append([sum(item[current:current + tmax]) + 872 for current in range(0, len(item), tmax)]) + 873 else: + 874 Q_sum.append([item[int(tmax / 2)]]) + 875 Q_top = [] + 876 if version in ['sfqcd']: + 877 for i in range(len(Q_sum) // (ncs + 1)): + 878 Q_top.append(Q_sum[i * (ncs + 1) + index_aim][0]) + 879 else: + 880 for i in range(len(Q) // dtr_cnfg): + 881 Q_top.append(Q_sum[dtr_cnfg * i][index_aim]) + 882 if len(Q_top) != len(traj_list) // dtr_cnfg: + 883 raise Exception("qtops and traj_list dont have the same length") + 884 + 885 if kwargs.get('integer_charge', False): + 886 Q_top = [round(q) for q in Q_top] + 887 + 888 truncated_file = file[:-len(postfix)] + 889 + 890 if "names" not in kwargs: + 891 try: + 892 idx = truncated_file.index('r') + 893 except Exception: + 894 if "names" not in kwargs: + 895 raise Exception("Automatic recognition of replicum failed, please enter the key word 'names'.") + 896 ens_name = truncated_file[:idx] + 897 rep_names.append(ens_name + '|' + truncated_file[idx:].split(".")[0]) + 898 else: + 899 names = kwargs.get("names") + 900 rep_names = names + 901 + 902 deltas.append(Q_top) + 903 + 904 rep_names = sort_names(rep_names) + 905 + 906 idl = [range(int(configlist[rep][r_start_index[rep]]), int(configlist[rep][r_stop_index[rep]]) + 1, 1) for rep in range(len(deltas))] + 907 deltas = [deltas[nrep][r_start_index[nrep]:r_stop_index[nrep] + 1] for nrep in range(len(deltas))] + 908 result = Obs(deltas, rep_names, idl=idl) + 909 result.tag = {"T": tmax - 1, + 910 "L": L} + 911 return result + 912 913 - 914 Q_sum = [] - 915 for i, item in enumerate(Q): - 916 if sum_t is True: - 917 Q_sum.append([sum(item[current:current + tmax]) - 918 for current in range(0, len(item), tmax)]) - 919 else: - 920 Q_sum.append([item[int(tmax / 2)]]) - 921 Q_top = [] - 922 if version in ['sfqcd']: - 923 for i in range(len(Q_sum) // (ncs + 1)): - 924 Q_top.append(Q_sum[i * (ncs + 1) + index_aim][0]) - 925 else: - 926 for i in range(len(Q) // dtr_cnfg): - 927 Q_top.append(Q_sum[dtr_cnfg * i][index_aim]) - 928 if len(Q_top) != len(traj_list) // dtr_cnfg: - 929 raise Exception("qtops and traj_list dont have the same length") - 930 - 931 if kwargs.get('integer_charge', False): - 932 Q_top = [round(q) for q in Q_top] - 933 - 934 truncated_file = file[:-len(postfix)] + 914def qtop_projection(qtop, target=0): + 915 """Returns the projection to the topological charge sector defined by target. + 916 + 917 Parameters + 918 ---------- + 919 path : Obs + 920 Topological charge. + 921 target : int + 922 Specifies the topological sector to be reweighted to (default 0) + 923 + 924 Returns + 925 ------- + 926 reto : Obs + 927 projection to the topological charge sector defined by target + 928 """ + 929 if qtop.reweighted: + 930 raise Exception('You can not use a reweighted observable for reweighting!') + 931 + 932 proj_qtop = [] + 933 for n in qtop.deltas: + 934 proj_qtop.append(np.array([1 if round(qtop.r_values[n] + q) == target else 0 for q in qtop.deltas[n]])) 935 - 936 if "names" not in kwargs: - 937 try: - 938 idx = truncated_file.index('r') - 939 except Exception: - 940 if "names" not in kwargs: - 941 raise Exception("Automatic recognition of replicum failed, please enter the key word 'names'.") - 942 ens_name = truncated_file[:idx] - 943 rep_names.append(ens_name + '|' + truncated_file[idx:].split(".")[0]) - 944 else: - 945 names = kwargs.get("names") - 946 rep_names = names - 947 - 948 deltas.append(Q_top) - 949 - 950 rep_names = sort_names(rep_names) - 951 - 952 idl = [range(int(configlist[rep][r_start_index[rep]]), int(configlist[rep][r_stop_index[rep]]) + 1, 1) for rep in range(len(deltas))] - 953 deltas = [deltas[nrep][r_start_index[nrep]:r_stop_index[nrep] + 1] for nrep in range(len(deltas))] - 954 result = Obs(deltas, rep_names, idl=idl) - 955 result.tag = {"T": tmax - 1, - 956 "L": L} - 957 return result - 958 - 959 - 960def qtop_projection(qtop, target=0): - 961 """Returns the projection to the topological charge sector defined by target. - 962 - 963 Parameters - 964 ---------- - 965 path : Obs - 966 Topological charge. - 967 target : int - 968 Specifies the topological sector to be reweighted to (default 0) - 969 - 970 Returns - 971 ------- - 972 reto : Obs - 973 projection to the topological charge sector defined by target - 974 """ - 975 if qtop.reweighted: - 976 raise Exception('You can not use a reweighted observable for reweighting!') - 977 - 978 proj_qtop = [] - 979 for n in qtop.deltas: - 980 proj_qtop.append(np.array([1 if round(qtop.r_values[n] + q) == target else 0 for q in qtop.deltas[n]])) - 981 - 982 reto = Obs(proj_qtop, qtop.names, idl=[qtop.idl[name] for name in qtop.names]) - 983 return reto - 984 - 985 - 986def read_qtop_sector(path, prefix, c, target=0, **kwargs): - 987 """Constructs reweighting factors to a specified topological sector. + 936 reto = Obs(proj_qtop, qtop.names, idl=[qtop.idl[name] for name in qtop.names]) + 937 return reto + 938 + 939 + 940def read_qtop_sector(path, prefix, c, target=0, **kwargs): + 941 """Constructs reweighting factors to a specified topological sector. + 942 + 943 Parameters + 944 ---------- + 945 path : str + 946 path of the measurement files + 947 prefix : str + 948 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat + 949 c : double + 950 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L + 951 target : int + 952 Specifies the topological sector to be reweighted to (default 0) + 953 dtr_cnfg : int + 954 (optional) parameter that specifies the number of trajectories + 955 between two configs. + 956 if it is not set, the distance between two measurements + 957 in the file is assumed to be the distance between two configurations. + 958 steps : int + 959 (optional) Distance between two configurations in units of trajectories / + 960 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given + 961 version : str + 962 version string of the openQCD (sfqcd) version used to create + 963 the ensemble. Default is 2.0. May also be set to sfqcd. + 964 L : int + 965 spatial length of the lattice in L/a. + 966 HAS to be set if version != sfqcd, since openQCD does not provide + 967 this in the header + 968 r_start : list + 969 offset of the first ensemble, making it easier to match + 970 later on with other Obs + 971 r_stop : list + 972 last configurations that need to be read (per replicum) + 973 files : list + 974 specify the exact files that need to be read + 975 from path, practical if e.g. only one replicum is needed + 976 names : list + 977 Alternative labeling for replicas/ensembles. + 978 Has to have the appropriate length + 979 Zeuthen_flow : bool + 980 (optional) If True, the Zeuthen flow is used for Qtop. Only possible + 981 for version=='sfqcd' If False, the Wilson flow is used. + 982 + 983 Returns + 984 ------- + 985 reto : Obs + 986 projection to the topological charge sector defined by target + 987 """ 988 - 989 Parameters - 990 ---------- - 991 path : str - 992 path of the measurement files - 993 prefix : str - 994 prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat - 995 c : double - 996 Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L - 997 target : int - 998 Specifies the topological sector to be reweighted to (default 0) - 999 dtr_cnfg : int -1000 (optional) parameter that specifies the number of trajectories -1001 between two configs. -1002 if it is not set, the distance between two measurements -1003 in the file is assumed to be the distance between two configurations. -1004 steps : int -1005 (optional) Distance between two configurations in units of trajectories / -1006 cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given -1007 version : str -1008 version string of the openQCD (sfqcd) version used to create -1009 the ensemble. Default is 2.0. May also be set to sfqcd. -1010 L : int -1011 spatial length of the lattice in L/a. -1012 HAS to be set if version != sfqcd, since openQCD does not provide -1013 this in the header -1014 r_start : list -1015 offset of the first ensemble, making it easier to match -1016 later on with other Obs -1017 r_stop : list -1018 last configurations that need to be read (per replicum) -1019 files : list -1020 specify the exact files that need to be read -1021 from path, practical if e.g. only one replicum is needed -1022 names : list -1023 Alternative labeling for replicas/ensembles. -1024 Has to have the appropriate length -1025 Zeuthen_flow : bool -1026 (optional) If True, the Zeuthen flow is used for Qtop. Only possible -1027 for version=='sfqcd' If False, the Wilson flow is used. -1028 -1029 Returns -1030 ------- -1031 reto : Obs -1032 projection to the topological charge sector defined by target -1033 """ -1034 -1035 if not isinstance(target, int): -1036 raise Exception("'target' has to be an integer.") + 989 if not isinstance(target, int): + 990 raise Exception("'target' has to be an integer.") + 991 + 992 kwargs['integer_charge'] = True + 993 qtop = read_qtop(path, prefix, c, **kwargs) + 994 + 995 return qtop_projection(qtop, target=target) + 996 + 997 + 998def read_ms5_xsf(path, prefix, qc, corr, sep="r", **kwargs): + 999 """ +1000 Read data from files in the specified directory with the specified prefix and quark combination extension, and return a `Corr` object containing the data. +1001 +1002 Parameters +1003 ---------- +1004 path : str +1005 The directory to search for the files in. +1006 prefix : str +1007 The prefix to match the files against. +1008 qc : str +1009 The quark combination extension to match the files against. +1010 corr : str +1011 The correlator to extract data for. +1012 sep : str, optional +1013 The separator to use when parsing the replika names. +1014 **kwargs +1015 Additional keyword arguments. The following keyword arguments are recognized: +1016 +1017 - names (List[str]): A list of names to use for the replicas. +1018 +1019 Returns +1020 ------- +1021 Corr +1022 A complex valued `Corr` object containing the data read from the files. In case of boudary to bulk correlators. +1023 or +1024 CObs +1025 A complex valued `CObs` object containing the data read from the files. In case of boudary to boundary correlators. +1026 +1027 +1028 Raises +1029 ------ +1030 FileNotFoundError +1031 If no files matching the specified prefix and quark combination extension are found in the specified directory. +1032 IOError +1033 If there is an error reading a file. +1034 struct.error +1035 If there is an error unpacking binary data. +1036 """ 1037 -1038 kwargs['integer_charge'] = True -1039 qtop = read_qtop(path, prefix, c, **kwargs) -1040 -1041 return qtop_projection(qtop, target=target) -1042 -1043 -1044def read_ms5_xsf(path, prefix, qc, corr, sep="r", **kwargs): -1045 """ -1046 Read data from files in the specified directory with the specified prefix and quark combination extension, and return a `Corr` object containing the data. -1047 -1048 Parameters -1049 ---------- -1050 path : str -1051 The directory to search for the files in. -1052 prefix : str -1053 The prefix to match the files against. -1054 qc : str -1055 The quark combination extension to match the files against. -1056 corr : str -1057 The correlator to extract data for. -1058 sep : str, optional -1059 The separator to use when parsing the replika names. -1060 **kwargs -1061 Additional keyword arguments. The following keyword arguments are recognized: -1062 -1063 - names (List[str]): A list of names to use for the replicas. -1064 -1065 Returns -1066 ------- -1067 Corr -1068 A complex valued `Corr` object containing the data read from the files. In case of boudary to bulk correlators. -1069 or -1070 CObs -1071 A complex valued `CObs` object containing the data read from the files. In case of boudary to boundary correlators. -1072 -1073 -1074 Raises -1075 ------ -1076 FileNotFoundError -1077 If no files matching the specified prefix and quark combination extension are found in the specified directory. -1078 IOError -1079 If there is an error reading a file. -1080 struct.error -1081 If there is an error unpacking binary data. -1082 """ -1083 -1084 # found = [] -1085 files = [] -1086 names = [] -1087 -1088 # test if the input is correct -1089 if qc not in ['dd', 'ud', 'du', 'uu']: -1090 raise Exception("Unknown quark conbination!") -1091 -1092 if corr not in ["gS", "gP", "gA", "gV", "gVt", "lA", "lV", "lVt", "lT", "lTt", "g1", "l1"]: -1093 raise Exception("Unknown correlator!") -1094 -1095 if "files" in kwargs: -1096 known_files = kwargs.get("files") -1097 else: -1098 known_files = [] -1099 files = _find_files(path, prefix, "ms5_xsf_" + qc, "dat", known_files=known_files) +1038 # found = [] +1039 files = [] +1040 names = [] +1041 +1042 # test if the input is correct +1043 if qc not in ['dd', 'ud', 'du', 'uu']: +1044 raise Exception("Unknown quark conbination!") +1045 +1046 if corr not in ["gS", "gP", "gA", "gV", "gVt", "lA", "lV", "lVt", "lT", "lTt", "g1", "l1"]: +1047 raise Exception("Unknown correlator!") +1048 +1049 if "files" in kwargs: +1050 known_files = kwargs.get("files") +1051 else: +1052 known_files = [] +1053 files = _find_files(path, prefix, "ms5_xsf_" + qc, "dat", known_files=known_files) +1054 +1055 if "names" in kwargs: +1056 names = kwargs.get("names") +1057 else: +1058 for f in files: +1059 if not sep == "": +1060 se = f.split(".")[0] +1061 for s in f.split(".")[1:-2]: +1062 se += "." + s +1063 names.append(se.split(sep)[0] + "|r" + se.split(sep)[1]) +1064 else: +1065 names.append(prefix) +1066 +1067 names = sorted(names) +1068 files = sorted(files) +1069 +1070 cnfgs = [] +1071 realsamples = [] +1072 imagsamples = [] +1073 repnum = 0 +1074 for file in files: +1075 with open(path + "/" + file, "rb") as fp: +1076 +1077 t = fp.read(8) +1078 kappa = struct.unpack('d', t)[0] +1079 t = fp.read(8) +1080 csw = struct.unpack('d', t)[0] +1081 t = fp.read(8) +1082 dF = struct.unpack('d', t)[0] +1083 t = fp.read(8) +1084 zF = struct.unpack('d', t)[0] +1085 +1086 t = fp.read(4) +1087 tmax = struct.unpack('i', t)[0] +1088 t = fp.read(4) +1089 bnd = struct.unpack('i', t)[0] +1090 +1091 placesBI = ["gS", "gP", +1092 "gA", "gV", +1093 "gVt", "lA", +1094 "lV", "lVt", +1095 "lT", "lTt"] +1096 placesBB = ["g1", "l1"] +1097 +1098 # the chunks have the following structure: +1099 # confignumber, 10x timedependent complex correlators as doubles, 2x timeindependent complex correlators as doubles 1100 -1101 if "names" in kwargs: -1102 names = kwargs.get("names") -1103 else: -1104 for f in files: -1105 if not sep == "": -1106 se = f.split(".")[0] -1107 for s in f.split(".")[1:-2]: -1108 se += "." + s -1109 names.append(se.split(sep)[0] + "|r" + se.split(sep)[1]) -1110 else: -1111 names.append(prefix) -1112 -1113 names = sorted(names) -1114 files = sorted(files) -1115 -1116 cnfgs = [] -1117 realsamples = [] -1118 imagsamples = [] -1119 repnum = 0 -1120 for file in files: -1121 with open(path + "/" + file, "rb") as fp: +1101 chunksize = 4 + (8 * 2 * tmax * 10) + (8 * 2 * 2) +1102 packstr = '=i' + ('d' * 2 * tmax * 10) + ('d' * 2 * 2) +1103 cnfgs.append([]) +1104 realsamples.append([]) +1105 imagsamples.append([]) +1106 for t in range(tmax): +1107 realsamples[repnum].append([]) +1108 imagsamples[repnum].append([]) +1109 +1110 while True: +1111 cnfgt = fp.read(chunksize) +1112 if not cnfgt: +1113 break +1114 asascii = struct.unpack(packstr, cnfgt) +1115 cnfg = asascii[0] +1116 cnfgs[repnum].append(cnfg) +1117 +1118 if corr not in placesBB: +1119 tmpcorr = asascii[1 + 2 * tmax * placesBI.index(corr):1 + 2 * tmax * placesBI.index(corr) + 2 * tmax] +1120 else: +1121 tmpcorr = asascii[1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr):1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr) + 2] 1122 -1123 t = fp.read(8) -1124 kappa = struct.unpack('d', t)[0] -1125 t = fp.read(8) -1126 csw = struct.unpack('d', t)[0] -1127 t = fp.read(8) -1128 dF = struct.unpack('d', t)[0] -1129 t = fp.read(8) -1130 zF = struct.unpack('d', t)[0] +1123 corrres = [[], []] +1124 for i in range(len(tmpcorr)): +1125 corrres[i % 2].append(tmpcorr[i]) +1126 for t in range(int(len(tmpcorr) / 2)): +1127 realsamples[repnum][t].append(corrres[0][t]) +1128 for t in range(int(len(tmpcorr) / 2)): +1129 imagsamples[repnum][t].append(corrres[1][t]) +1130 repnum += 1 1131 -1132 t = fp.read(4) -1133 tmax = struct.unpack('i', t)[0] -1134 t = fp.read(4) -1135 bnd = struct.unpack('i', t)[0] -1136 -1137 placesBI = ["gS", "gP", -1138 "gA", "gV", -1139 "gVt", "lA", -1140 "lV", "lVt", -1141 "lT", "lTt"] -1142 placesBB = ["g1", "l1"] -1143 -1144 # the chunks have the following structure: -1145 # confignumber, 10x timedependent complex correlators as doubles, 2x timeindependent complex correlators as doubles +1132 s = "Read correlator " + corr + " from " + str(repnum) + " replika with " + str(len(realsamples[0][t])) +1133 for rep in range(1, repnum): +1134 s += ", " + str(len(realsamples[rep][t])) +1135 s += " samples" +1136 print(s) +1137 print("Asserted run parameters:\n T:", tmax, "kappa:", kappa, "csw:", csw, "dF:", dF, "zF:", zF, "bnd:", bnd) +1138 +1139 # we have the data now... but we need to re format the whole thing and put it into Corr objects. +1140 +1141 compObs = [] +1142 +1143 for t in range(int(len(tmpcorr) / 2)): +1144 compObs.append(CObs(Obs([realsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs), +1145 Obs([imagsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs))) 1146 -1147 chunksize = 4 + (8 * 2 * tmax * 10) + (8 * 2 * 2) -1148 packstr = '=i' + ('d' * 2 * tmax * 10) + ('d' * 2 * 2) -1149 cnfgs.append([]) -1150 realsamples.append([]) -1151 imagsamples.append([]) -1152 for t in range(tmax): -1153 realsamples[repnum].append([]) -1154 imagsamples[repnum].append([]) -1155 -1156 while True: -1157 cnfgt = fp.read(chunksize) -1158 if not cnfgt: -1159 break -1160 asascii = struct.unpack(packstr, cnfgt) -1161 cnfg = asascii[0] -1162 cnfgs[repnum].append(cnfg) -1163 -1164 if corr not in placesBB: -1165 tmpcorr = asascii[1 + 2 * tmax * placesBI.index(corr):1 + 2 * tmax * placesBI.index(corr) + 2 * tmax] -1166 else: -1167 tmpcorr = asascii[1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr):1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr) + 2] -1168 -1169 corrres = [[], []] -1170 for i in range(len(tmpcorr)): -1171 corrres[i % 2].append(tmpcorr[i]) -1172 for t in range(int(len(tmpcorr) / 2)): -1173 realsamples[repnum][t].append(corrres[0][t]) -1174 for t in range(int(len(tmpcorr) / 2)): -1175 imagsamples[repnum][t].append(corrres[1][t]) -1176 repnum += 1 -1177 -1178 s = "Read correlator " + corr + " from " + str(repnum) + " replika with " + str(len(realsamples[0][t])) -1179 for rep in range(1, repnum): -1180 s += ", " + str(len(realsamples[rep][t])) -1181 s += " samples" -1182 print(s) -1183 print("Asserted run parameters:\n T:", tmax, "kappa:", kappa, "csw:", csw, "dF:", dF, "zF:", zF, "bnd:", bnd) -1184 -1185 # we have the data now... but we need to re format the whole thing and put it into Corr objects. -1186 -1187 compObs = [] -1188 -1189 for t in range(int(len(tmpcorr) / 2)): -1190 compObs.append(CObs(Obs([realsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs), -1191 Obs([imagsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs))) -1192 -1193 if len(compObs) == 1: -1194 return compObs[0] -1195 else: -1196 return Corr(compObs) +1147 if len(compObs) == 1: +1148 return compObs[0] +1149 else: +1150 return Corr(compObs)
    @@ -1305,223 +1259,223 @@ -
     16def read_rwms(path, prefix, version='2.0', names=None, **kwargs):
    - 17    """Read rwms format from given folder structure. Returns a list of length nrw
    - 18
    - 19    Parameters
    - 20    ----------
    - 21    path : str
    - 22        path that contains the data files
    - 23    prefix : str
    - 24        all files in path that start with prefix are considered as input files.
    - 25        May be used together postfix to consider only special file endings.
    - 26        Prefix is ignored, if the keyword 'files' is used.
    - 27    version : str
    - 28        version of openQCD, default 2.0
    - 29    names : list
    - 30        list of names that is assigned to the data according according
    - 31        to the order in the file list. Use careful, if you do not provide file names!
    - 32    r_start : list
    - 33        list which contains the first config to be read for each replicum
    - 34    r_stop : list
    - 35        list which contains the last config to be read for each replicum
    - 36    r_step : int
    - 37        integer that defines a fixed step size between two measurements (in units of configs)
    - 38        If not given, r_step=1 is assumed.
    - 39    postfix : str
    - 40        postfix of the file to read, e.g. '.ms1' for openQCD-files
    - 41    files : list
    - 42        list which contains the filenames to be read. No automatic detection of
    - 43        files performed if given.
    - 44    print_err : bool
    - 45        Print additional information that is useful for debugging.
    - 46
    - 47    Returns
    - 48    -------
    - 49    rwms : Obs
    - 50        Reweighting factors read
    - 51    """
    - 52    known_oqcd_versions = ['1.4', '1.6', '2.0']
    - 53    if not (version in known_oqcd_versions):
    - 54        raise Exception('Unknown openQCD version defined!')
    - 55    print("Working with openQCD version " + version)
    - 56    if 'postfix' in kwargs:
    - 57        postfix = kwargs.get('postfix')
    - 58    else:
    - 59        postfix = ''
    - 60
    - 61    if 'files' in kwargs:
    - 62        known_files = kwargs.get('files')
    - 63    else:
    - 64        known_files = []
    +            
     14def read_rwms(path, prefix, version='2.0', names=None, **kwargs):
    + 15    """Read rwms format from given folder structure. Returns a list of length nrw
    + 16
    + 17    Parameters
    + 18    ----------
    + 19    path : str
    + 20        path that contains the data files
    + 21    prefix : str
    + 22        all files in path that start with prefix are considered as input files.
    + 23        May be used together postfix to consider only special file endings.
    + 24        Prefix is ignored, if the keyword 'files' is used.
    + 25    version : str
    + 26        version of openQCD, default 2.0
    + 27    names : list
    + 28        list of names that is assigned to the data according according
    + 29        to the order in the file list. Use careful, if you do not provide file names!
    + 30    r_start : list
    + 31        list which contains the first config to be read for each replicum
    + 32    r_stop : list
    + 33        list which contains the last config to be read for each replicum
    + 34    r_step : int
    + 35        integer that defines a fixed step size between two measurements (in units of configs)
    + 36        If not given, r_step=1 is assumed.
    + 37    postfix : str
    + 38        postfix of the file to read, e.g. '.ms1' for openQCD-files
    + 39    files : list
    + 40        list which contains the filenames to be read. No automatic detection of
    + 41        files performed if given.
    + 42    print_err : bool
    + 43        Print additional information that is useful for debugging.
    + 44
    + 45    Returns
    + 46    -------
    + 47    rwms : Obs
    + 48        Reweighting factors read
    + 49    """
    + 50    known_oqcd_versions = ['1.4', '1.6', '2.0']
    + 51    if not (version in known_oqcd_versions):
    + 52        raise Exception('Unknown openQCD version defined!')
    + 53    print("Working with openQCD version " + version)
    + 54    if 'postfix' in kwargs:
    + 55        postfix = kwargs.get('postfix')
    + 56    else:
    + 57        postfix = ''
    + 58
    + 59    if 'files' in kwargs:
    + 60        known_files = kwargs.get('files')
    + 61    else:
    + 62        known_files = []
    + 63
    + 64    ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files)
      65
    - 66    ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files)
    + 66    replica = len(ls)
      67
    - 68    replica = len(ls)
    - 69
    - 70    if 'r_start' in kwargs:
    - 71        r_start = kwargs.get('r_start')
    - 72        if len(r_start) != replica:
    - 73            raise Exception('r_start does not match number of replicas')
    - 74        r_start = [o if o else None for o in r_start]
    - 75    else:
    - 76        r_start = [None] * replica
    - 77
    - 78    if 'r_stop' in kwargs:
    - 79        r_stop = kwargs.get('r_stop')
    - 80        if len(r_stop) != replica:
    - 81            raise Exception('r_stop does not match number of replicas')
    - 82    else:
    - 83        r_stop = [None] * replica
    - 84
    - 85    if 'r_step' in kwargs:
    - 86        r_step = kwargs.get('r_step')
    - 87    else:
    - 88        r_step = 1
    - 89
    - 90    print('Read reweighting factors from', prefix[:-1], ',',
    - 91          replica, 'replica', end='')
    - 92
    - 93    if names is None:
    - 94        rep_names = []
    - 95        for entry in ls:
    - 96            truncated_entry = entry
    - 97            suffixes = [".dat", ".rwms", ".ms1"]
    - 98            for suffix in suffixes:
    - 99                if truncated_entry.endswith(suffix):
    -100                    truncated_entry = truncated_entry[0:-len(suffix)]
    -101            idx = truncated_entry.index('r')
    -102            rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    -103    else:
    -104        rep_names = names
    + 68    if 'r_start' in kwargs:
    + 69        r_start = kwargs.get('r_start')
    + 70        if len(r_start) != replica:
    + 71            raise Exception('r_start does not match number of replicas')
    + 72        r_start = [o if o else None for o in r_start]
    + 73    else:
    + 74        r_start = [None] * replica
    + 75
    + 76    if 'r_stop' in kwargs:
    + 77        r_stop = kwargs.get('r_stop')
    + 78        if len(r_stop) != replica:
    + 79            raise Exception('r_stop does not match number of replicas')
    + 80    else:
    + 81        r_stop = [None] * replica
    + 82
    + 83    if 'r_step' in kwargs:
    + 84        r_step = kwargs.get('r_step')
    + 85    else:
    + 86        r_step = 1
    + 87
    + 88    print('Read reweighting factors from', prefix[:-1], ',',
    + 89          replica, 'replica', end='')
    + 90
    + 91    if names is None:
    + 92        rep_names = []
    + 93        for entry in ls:
    + 94            truncated_entry = entry
    + 95            suffixes = [".dat", ".rwms", ".ms1"]
    + 96            for suffix in suffixes:
    + 97                if truncated_entry.endswith(suffix):
    + 98                    truncated_entry = truncated_entry[0:-len(suffix)]
    + 99            idx = truncated_entry.index('r')
    +100            rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    +101    else:
    +102        rep_names = names
    +103
    +104    rep_names = sort_names(rep_names)
     105
    -106    rep_names = sort_names(rep_names)
    -107
    -108    print_err = 0
    -109    if 'print_err' in kwargs:
    -110        print_err = 1
    -111        print()
    +106    print_err = 0
    +107    if 'print_err' in kwargs:
    +108        print_err = 1
    +109        print()
    +110
    +111    deltas = []
     112
    -113    deltas = []
    -114
    -115    configlist = []
    -116    r_start_index = []
    -117    r_stop_index = []
    -118
    -119    for rep in range(replica):
    -120        tmp_array = []
    -121        with open(path + '/' + ls[rep], 'rb') as fp:
    -122
    -123            t = fp.read(4)  # number of reweighting factors
    -124            if rep == 0:
    -125                nrw = struct.unpack('i', t)[0]
    -126                if version == '2.0':
    -127                    nrw = int(nrw / 2)
    -128                for k in range(nrw):
    -129                    deltas.append([])
    -130            else:
    -131                if ((nrw != struct.unpack('i', t)[0] and (not version == '2.0')) or (nrw != struct.unpack('i', t)[0] / 2 and version == '2.0')):
    -132                    raise Exception('Error: different number of reweighting factors for replicum', rep)
    -133
    -134            for k in range(nrw):
    -135                tmp_array.append([])
    -136
    -137            # This block is necessary for openQCD1.6 and openQCD2.0 ms1 files
    -138            nfct = []
    -139            if version in ['1.6', '2.0']:
    -140                for i in range(nrw):
    -141                    t = fp.read(4)
    -142                    nfct.append(struct.unpack('i', t)[0])
    -143            else:
    -144                for i in range(nrw):
    -145                    nfct.append(1)
    -146
    -147            nsrc = []
    -148            for i in range(nrw):
    -149                t = fp.read(4)
    -150                nsrc.append(struct.unpack('i', t)[0])
    -151            if version == '2.0':
    -152                if not struct.unpack('i', fp.read(4))[0] == 0:
    -153                    raise Exception("You are using the input for openQCD version 2.0, this is not correct.")
    -154
    -155            configlist.append([])
    -156            while True:
    -157                t = fp.read(4)
    -158                if len(t) < 4:
    -159                    break
    -160                config_no = struct.unpack('i', t)[0]
    -161                configlist[-1].append(config_no)
    -162                for i in range(nrw):
    -163                    if (version == '2.0'):
    -164                        tmpd = _read_array_openQCD2(fp)
    -165                        tmpd = _read_array_openQCD2(fp)
    -166                        tmp_rw = tmpd['arr']
    -167                        tmp_nfct = 1.0
    -168                        for j in range(tmpd['n'][0]):
    -169                            tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw[j])))
    -170                            if print_err:
    -171                                print(config_no, i, j,
    -172                                      np.mean(np.exp(-np.asarray(tmp_rw[j]))),
    -173                                      np.std(np.exp(-np.asarray(tmp_rw[j]))))
    -174                                print('Sources:',
    -175                                      np.exp(-np.asarray(tmp_rw[j])))
    -176                                print('Partial factor:', tmp_nfct)
    -177                    elif version == '1.6' or version == '1.4':
    -178                        tmp_nfct = 1.0
    -179                        for j in range(nfct[i]):
    -180                            t = fp.read(8 * nsrc[i])
    -181                            t = fp.read(8 * nsrc[i])
    -182                            tmp_rw = struct.unpack('d' * nsrc[i], t)
    -183                            tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw)))
    -184                            if print_err:
    -185                                print(config_no, i, j,
    -186                                      np.mean(np.exp(-np.asarray(tmp_rw))),
    -187                                      np.std(np.exp(-np.asarray(tmp_rw))))
    -188                                print('Sources:', np.exp(-np.asarray(tmp_rw)))
    -189                                print('Partial factor:', tmp_nfct)
    -190                    tmp_array[i].append(tmp_nfct)
    -191
    -192            diffmeas = configlist[-1][-1] - configlist[-1][-2]
    -193            configlist[-1] = [item // diffmeas for item in configlist[-1]]
    -194            if configlist[-1][0] > 1 and diffmeas > 1:
    -195                warnings.warn('Assume thermalization and that the first measurement belongs to the first config.')
    -196                offset = configlist[-1][0] - 1
    -197                configlist[-1] = [item - offset for item in configlist[-1]]
    -198
    -199            if r_start[rep] is None:
    -200                r_start_index.append(0)
    -201            else:
    -202                try:
    -203                    r_start_index.append(configlist[-1].index(r_start[rep]))
    -204                except ValueError:
    -205                    raise Exception('Config %d not in file with range [%d, %d]' % (
    -206                        r_start[rep], configlist[-1][0], configlist[-1][-1])) from None
    -207
    -208            if r_stop[rep] is None:
    -209                r_stop_index.append(len(configlist[-1]) - 1)
    -210            else:
    -211                try:
    -212                    r_stop_index.append(configlist[-1].index(r_stop[rep]))
    -213                except ValueError:
    -214                    raise Exception('Config %d not in file with range [%d, %d]' % (
    -215                        r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None
    -216
    -217            for k in range(nrw):
    -218                deltas[k].append(tmp_array[k][r_start_index[rep]:r_stop_index[rep] + 1][::r_step])
    -219
    -220    if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]):
    -221        raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist])
    -222    stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist]
    -223    if np.any([step != 1 for step in stepsizes]):
    -224        warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning)
    -225
    -226    print(',', nrw, 'reweighting factors with', nsrc, 'sources')
    -227    result = []
    -228    idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)]
    -229
    -230    for t in range(nrw):
    -231        result.append(Obs(deltas[t], rep_names, idl=idl))
    -232    return result
    +113    configlist = []
    +114    r_start_index = []
    +115    r_stop_index = []
    +116
    +117    for rep in range(replica):
    +118        tmp_array = []
    +119        with open(path + '/' + ls[rep], 'rb') as fp:
    +120
    +121            t = fp.read(4)  # number of reweighting factors
    +122            if rep == 0:
    +123                nrw = struct.unpack('i', t)[0]
    +124                if version == '2.0':
    +125                    nrw = int(nrw / 2)
    +126                for k in range(nrw):
    +127                    deltas.append([])
    +128            else:
    +129                if ((nrw != struct.unpack('i', t)[0] and (not version == '2.0')) or (nrw != struct.unpack('i', t)[0] / 2 and version == '2.0')):
    +130                    raise Exception('Error: different number of reweighting factors for replicum', rep)
    +131
    +132            for k in range(nrw):
    +133                tmp_array.append([])
    +134
    +135            # This block is necessary for openQCD1.6 and openQCD2.0 ms1 files
    +136            nfct = []
    +137            if version in ['1.6', '2.0']:
    +138                for i in range(nrw):
    +139                    t = fp.read(4)
    +140                    nfct.append(struct.unpack('i', t)[0])
    +141            else:
    +142                for i in range(nrw):
    +143                    nfct.append(1)
    +144
    +145            nsrc = []
    +146            for i in range(nrw):
    +147                t = fp.read(4)
    +148                nsrc.append(struct.unpack('i', t)[0])
    +149            if version == '2.0':
    +150                if not struct.unpack('i', fp.read(4))[0] == 0:
    +151                    raise Exception("You are using the input for openQCD version 2.0, this is not correct.")
    +152
    +153            configlist.append([])
    +154            while True:
    +155                t = fp.read(4)
    +156                if len(t) < 4:
    +157                    break
    +158                config_no = struct.unpack('i', t)[0]
    +159                configlist[-1].append(config_no)
    +160                for i in range(nrw):
    +161                    if (version == '2.0'):
    +162                        tmpd = _read_array_openQCD2(fp)
    +163                        tmpd = _read_array_openQCD2(fp)
    +164                        tmp_rw = tmpd['arr']
    +165                        tmp_nfct = 1.0
    +166                        for j in range(tmpd['n'][0]):
    +167                            tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw[j])))
    +168                            if print_err:
    +169                                print(config_no, i, j,
    +170                                      np.mean(np.exp(-np.asarray(tmp_rw[j]))),
    +171                                      np.std(np.exp(-np.asarray(tmp_rw[j]))))
    +172                                print('Sources:',
    +173                                      np.exp(-np.asarray(tmp_rw[j])))
    +174                                print('Partial factor:', tmp_nfct)
    +175                    elif version == '1.6' or version == '1.4':
    +176                        tmp_nfct = 1.0
    +177                        for j in range(nfct[i]):
    +178                            t = fp.read(8 * nsrc[i])
    +179                            t = fp.read(8 * nsrc[i])
    +180                            tmp_rw = struct.unpack('d' * nsrc[i], t)
    +181                            tmp_nfct *= np.mean(np.exp(-np.asarray(tmp_rw)))
    +182                            if print_err:
    +183                                print(config_no, i, j,
    +184                                      np.mean(np.exp(-np.asarray(tmp_rw))),
    +185                                      np.std(np.exp(-np.asarray(tmp_rw))))
    +186                                print('Sources:', np.exp(-np.asarray(tmp_rw)))
    +187                                print('Partial factor:', tmp_nfct)
    +188                    tmp_array[i].append(tmp_nfct)
    +189
    +190            diffmeas = configlist[-1][-1] - configlist[-1][-2]
    +191            configlist[-1] = [item // diffmeas for item in configlist[-1]]
    +192            if configlist[-1][0] > 1 and diffmeas > 1:
    +193                warnings.warn('Assume thermalization and that the first measurement belongs to the first config.')
    +194                offset = configlist[-1][0] - 1
    +195                configlist[-1] = [item - offset for item in configlist[-1]]
    +196
    +197            if r_start[rep] is None:
    +198                r_start_index.append(0)
    +199            else:
    +200                try:
    +201                    r_start_index.append(configlist[-1].index(r_start[rep]))
    +202                except ValueError:
    +203                    raise Exception('Config %d not in file with range [%d, %d]' % (
    +204                        r_start[rep], configlist[-1][0], configlist[-1][-1])) from None
    +205
    +206            if r_stop[rep] is None:
    +207                r_stop_index.append(len(configlist[-1]) - 1)
    +208            else:
    +209                try:
    +210                    r_stop_index.append(configlist[-1].index(r_stop[rep]))
    +211                except ValueError:
    +212                    raise Exception('Config %d not in file with range [%d, %d]' % (
    +213                        r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None
    +214
    +215            for k in range(nrw):
    +216                deltas[k].append(tmp_array[k][r_start_index[rep]:r_stop_index[rep] + 1][::r_step])
    +217
    +218    if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]):
    +219        raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist])
    +220    stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist]
    +221    if np.any([step != 1 for step in stepsizes]):
    +222        warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning)
    +223
    +224    print(',', nrw, 'reweighting factors with', nsrc, 'sources')
    +225    result = []
    +226    idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)]
    +227
    +228    for t in range(nrw):
    +229        result.append(Obs(deltas[t], rep_names, idl=idl))
    +230    return result
     
    @@ -1578,248 +1532,204 @@ Reweighting factors read
    -
    235def extract_t0(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, postfix='ms', **kwargs):
    -236    """Extract t0 from given .ms.dat files. Returns t0 as Obs.
    -237
    -238    It is assumed that all boundary effects have
    -239    sufficiently decayed at x0=xmin.
    -240    The data around the zero crossing of t^2<E> - 0.3
    -241    is fitted with a linear function
    -242    from which the exact root is extracted.
    -243
    -244    It is assumed that one measurement is performed for each config.
    -245    If this is not the case, the resulting idl, as well as the handling
    -246    of r_start, r_stop and r_step is wrong and the user has to correct
    -247    this in the resulting observable.
    -248
    -249    Parameters
    -250    ----------
    -251    path : str
    -252        Path to .ms.dat files
    -253    prefix : str
    -254        Ensemble prefix
    -255    dtr_read : int
    -256        Determines how many trajectories should be skipped
    -257        when reading the ms.dat files.
    -258        Corresponds to dtr_cnfg / dtr_ms in the openQCD input file.
    -259    xmin : int
    -260        First timeslice where the boundary
    -261        effects have sufficiently decayed.
    -262    spatial_extent : int
    -263        spatial extent of the lattice, required for normalization.
    -264    fit_range : int
    -265        Number of data points left and right of the zero
    -266        crossing to be included in the linear fit. (Default: 5)
    -267    postfix : str
    -268        Postfix of measurement file (Default: ms)
    -269    r_start : list
    -270        list which contains the first config to be read for each replicum.
    -271    r_stop : list
    -272        list which contains the last config to be read for each replicum.
    -273    r_step : int
    -274        integer that defines a fixed step size between two measurements (in units of configs)
    -275        If not given, r_step=1 is assumed.
    -276    plaquette : bool
    -277        If true extract the plaquette estimate of t0 instead.
    -278    names : list
    -279        list of names that is assigned to the data according according
    -280        to the order in the file list. Use careful, if you do not provide file names!
    -281    files : list
    -282        list which contains the filenames to be read. No automatic detection of
    -283        files performed if given.
    -284    plot_fit : bool
    -285        If true, the fit for the extraction of t0 is shown together with the data.
    -286    assume_thermalization : bool
    -287        If True: If the first record divided by the distance between two measurements is larger than
    -288        1, it is assumed that this is due to thermalization and the first measurement belongs
    -289        to the first config (default).
    -290        If False: The config numbers are assumed to be traj_number // difference
    -291
    -292    Returns
    -293    -------
    -294    t0 : Obs
    -295        Extracted t0
    -296    """
    -297
    -298    if 'files' in kwargs:
    -299        known_files = kwargs.get('files')
    -300    else:
    -301        known_files = []
    +            
    233def extract_t0(path, prefix, dtr_read, xmin, spatial_extent, fit_range=5, postfix='ms', **kwargs):
    +234    """Extract t0 from given .ms.dat files. Returns t0 as Obs.
    +235
    +236    It is assumed that all boundary effects have
    +237    sufficiently decayed at x0=xmin.
    +238    The data around the zero crossing of t^2<E> - 0.3
    +239    is fitted with a linear function
    +240    from which the exact root is extracted.
    +241
    +242    It is assumed that one measurement is performed for each config.
    +243    If this is not the case, the resulting idl, as well as the handling
    +244    of r_start, r_stop and r_step is wrong and the user has to correct
    +245    this in the resulting observable.
    +246
    +247    Parameters
    +248    ----------
    +249    path : str
    +250        Path to .ms.dat files
    +251    prefix : str
    +252        Ensemble prefix
    +253    dtr_read : int
    +254        Determines how many trajectories should be skipped
    +255        when reading the ms.dat files.
    +256        Corresponds to dtr_cnfg / dtr_ms in the openQCD input file.
    +257    xmin : int
    +258        First timeslice where the boundary
    +259        effects have sufficiently decayed.
    +260    spatial_extent : int
    +261        spatial extent of the lattice, required for normalization.
    +262    fit_range : int
    +263        Number of data points left and right of the zero
    +264        crossing to be included in the linear fit. (Default: 5)
    +265    postfix : str
    +266        Postfix of measurement file (Default: ms)
    +267    r_start : list
    +268        list which contains the first config to be read for each replicum.
    +269    r_stop : list
    +270        list which contains the last config to be read for each replicum.
    +271    r_step : int
    +272        integer that defines a fixed step size between two measurements (in units of configs)
    +273        If not given, r_step=1 is assumed.
    +274    plaquette : bool
    +275        If true extract the plaquette estimate of t0 instead.
    +276    names : list
    +277        list of names that is assigned to the data according according
    +278        to the order in the file list. Use careful, if you do not provide file names!
    +279    files : list
    +280        list which contains the filenames to be read. No automatic detection of
    +281        files performed if given.
    +282    plot_fit : bool
    +283        If true, the fit for the extraction of t0 is shown together with the data.
    +284    assume_thermalization : bool
    +285        If True: If the first record divided by the distance between two measurements is larger than
    +286        1, it is assumed that this is due to thermalization and the first measurement belongs
    +287        to the first config (default).
    +288        If False: The config numbers are assumed to be traj_number // difference
    +289
    +290    Returns
    +291    -------
    +292    t0 : Obs
    +293        Extracted t0
    +294    """
    +295
    +296    if 'files' in kwargs:
    +297        known_files = kwargs.get('files')
    +298    else:
    +299        known_files = []
    +300
    +301    ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files)
     302
    -303    ls = _find_files(path, prefix, postfix, 'dat', known_files=known_files)
    +303    replica = len(ls)
     304
    -305    replica = len(ls)
    -306
    -307    if 'r_start' in kwargs:
    -308        r_start = kwargs.get('r_start')
    -309        if len(r_start) != replica:
    -310            raise Exception('r_start does not match number of replicas')
    -311        r_start = [o if o else None for o in r_start]
    -312    else:
    -313        r_start = [None] * replica
    -314
    -315    if 'r_stop' in kwargs:
    -316        r_stop = kwargs.get('r_stop')
    -317        if len(r_stop) != replica:
    -318            raise Exception('r_stop does not match number of replicas')
    -319    else:
    -320        r_stop = [None] * replica
    -321
    -322    if 'r_step' in kwargs:
    -323        r_step = kwargs.get('r_step')
    -324    else:
    -325        r_step = 1
    +305    if 'r_start' in kwargs:
    +306        r_start = kwargs.get('r_start')
    +307        if len(r_start) != replica:
    +308            raise Exception('r_start does not match number of replicas')
    +309        r_start = [o if o else None for o in r_start]
    +310    else:
    +311        r_start = [None] * replica
    +312
    +313    if 'r_stop' in kwargs:
    +314        r_stop = kwargs.get('r_stop')
    +315        if len(r_stop) != replica:
    +316            raise Exception('r_stop does not match number of replicas')
    +317    else:
    +318        r_stop = [None] * replica
    +319
    +320    if 'r_step' in kwargs:
    +321        r_step = kwargs.get('r_step')
    +322    else:
    +323        r_step = 1
    +324
    +325    print('Extract t0 from', prefix, ',', replica, 'replica')
     326
    -327    print('Extract t0 from', prefix, ',', replica, 'replica')
    -328
    -329    if 'names' in kwargs:
    -330        rep_names = kwargs.get('names')
    -331    else:
    -332        rep_names = []
    -333        for entry in ls:
    -334            truncated_entry = entry.split('.')[0]
    -335            idx = truncated_entry.index('r')
    -336            rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    +327    if 'names' in kwargs:
    +328        rep_names = kwargs.get('names')
    +329    else:
    +330        rep_names = []
    +331        for entry in ls:
    +332            truncated_entry = entry.split('.')[0]
    +333            idx = truncated_entry.index('r')
    +334            rep_names.append(truncated_entry[:idx] + '|' + truncated_entry[idx:])
    +335
    +336    Ysum = []
     337
    -338    Ysum = []
    -339
    -340    configlist = []
    -341    r_start_index = []
    -342    r_stop_index = []
    +338    configlist = []
    +339    r_start_index = []
    +340    r_stop_index = []
    +341
    +342    for rep in range(replica):
     343
    -344    for rep in range(replica):
    -345
    -346        with open(path + '/' + ls[rep], 'rb') as fp:
    -347            t = fp.read(12)
    -348            header = struct.unpack('iii', t)
    -349            if rep == 0:
    -350                dn = header[0]
    -351                nn = header[1]
    -352                tmax = header[2]
    -353            elif dn != header[0] or nn != header[1] or tmax != header[2]:
    -354                raise Exception('Replica parameters do not match.')
    -355
    -356            t = fp.read(8)
    -357            if rep == 0:
    -358                eps = struct.unpack('d', t)[0]
    -359                print('Step size:', eps, ', Maximal t value:', dn * (nn) * eps)
    -360            elif eps != struct.unpack('d', t)[0]:
    -361                raise Exception('Values for eps do not match among replica.')
    +344        with open(path + '/' + ls[rep], 'rb') as fp:
    +345            t = fp.read(12)
    +346            header = struct.unpack('iii', t)
    +347            if rep == 0:
    +348                dn = header[0]
    +349                nn = header[1]
    +350                tmax = header[2]
    +351            elif dn != header[0] or nn != header[1] or tmax != header[2]:
    +352                raise Exception('Replica parameters do not match.')
    +353
    +354            t = fp.read(8)
    +355            if rep == 0:
    +356                eps = struct.unpack('d', t)[0]
    +357                print('Step size:', eps, ', Maximal t value:', dn * (nn) * eps)
    +358            elif eps != struct.unpack('d', t)[0]:
    +359                raise Exception('Values for eps do not match among replica.')
    +360
    +361            Ysl = []
     362
    -363            Ysl = []
    -364
    -365            configlist.append([])
    -366            while True:
    -367                t = fp.read(4)
    -368                if (len(t) < 4):
    -369                    break
    -370                nc = struct.unpack('i', t)[0]
    -371                configlist[-1].append(nc)
    -372
    -373                t = fp.read(8 * tmax * (nn + 1))
    -374                if kwargs.get('plaquette'):
    -375                    if nc % dtr_read == 0:
    -376                        Ysl.append(struct.unpack('d' * tmax * (nn + 1), t))
    -377                t = fp.read(8 * tmax * (nn + 1))
    -378                if not kwargs.get('plaquette'):
    -379                    if nc % dtr_read == 0:
    -380                        Ysl.append(struct.unpack('d' * tmax * (nn + 1), t))
    -381                t = fp.read(8 * tmax * (nn + 1))
    -382
    -383        Ysum.append([])
    -384        for i, item in enumerate(Ysl):
    -385            Ysum[-1].append([np.mean(item[current + xmin:
    -386                             current + tmax - xmin])
    -387                            for current in range(0, len(item), tmax)])
    -388
    -389        diffmeas = configlist[-1][-1] - configlist[-1][-2]
    -390        configlist[-1] = [item // diffmeas for item in configlist[-1]]
    -391        if kwargs.get('assume_thermalization', True) and configlist[-1][0] > 1:
    -392            warnings.warn('Assume thermalization and that the first measurement belongs to the first config.')
    -393            offset = configlist[-1][0] - 1
    -394            configlist[-1] = [item - offset for item in configlist[-1]]
    -395
    -396        if r_start[rep] is None:
    -397            r_start_index.append(0)
    -398        else:
    -399            try:
    -400                r_start_index.append(configlist[-1].index(r_start[rep]))
    -401            except ValueError:
    -402                raise Exception('Config %d not in file with range [%d, %d]' % (
    -403                    r_start[rep], configlist[-1][0], configlist[-1][-1])) from None
    -404
    -405        if r_stop[rep] is None:
    -406            r_stop_index.append(len(configlist[-1]) - 1)
    -407        else:
    -408            try:
    -409                r_stop_index.append(configlist[-1].index(r_stop[rep]))
    -410            except ValueError:
    -411                raise Exception('Config %d not in file with range [%d, %d]' % (
    -412                    r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None
    -413
    -414    if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]):
    -415        raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist])
    -416    stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist]
    -417    if np.any([step != 1 for step in stepsizes]):
    -418        warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning)
    -419
    -420    idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)]
    -421    t2E_dict = {}
    -422    for n in range(nn + 1):
    -423        samples = []
    -424        for nrep, rep in enumerate(Ysum):
    -425            samples.append([])
    -426            for cnfg in rep:
    -427                samples[-1].append(cnfg[n])
    -428            samples[-1] = samples[-1][r_start_index[nrep]:r_stop_index[nrep] + 1][::r_step]
    -429        new_obs = Obs(samples, rep_names, idl=idl)
    -430        t2E_dict[n * dn * eps] = (n * dn * eps) ** 2 * new_obs / (spatial_extent ** 3) - 0.3
    -431
    -432    zero_crossing = np.argmax(np.array(
    -433        [o.value for o in t2E_dict.values()]) > 0.0)
    -434
    -435    x = list(t2E_dict.keys())[zero_crossing - fit_range:
    -436                              zero_crossing + fit_range]
    -437    y = list(t2E_dict.values())[zero_crossing - fit_range:
    -438                                zero_crossing + fit_range]
    -439    [o.gamma_method() for o in y]
    -440
    -441    fit_result = fit_lin(x, y)
    -442
    -443    if kwargs.get('plot_fit'):
    -444        plt.figure()
    -445        gs = gridspec.GridSpec(2, 1, height_ratios=[3, 1], wspace=0.0, hspace=0.0)
    -446        ax0 = plt.subplot(gs[0])
    -447        xmore = list(t2E_dict.keys())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2]
    -448        ymore = list(t2E_dict.values())[zero_crossing - fit_range - 2: zero_crossing + fit_range + 2]
    -449        [o.gamma_method() for o in ymore]
    -450        ax0.errorbar(xmore, [yi.value for yi in ymore], yerr=[yi.dvalue for yi in ymore], fmt='x')
    -451        xplot = np.linspace(np.min(x), np.max(x))
    -452        yplot = [fit_result[0] + fit_result[1] * xi for xi in xplot]
    -453        [yi.gamma_method() for yi in yplot]
    -454        ax0.fill_between(xplot, y1=[yi.value - yi.dvalue for yi in yplot], y2=[yi.value + yi.dvalue for yi in yplot])
    -455        retval = (-fit_result[0] / fit_result[1])
    -456        retval.gamma_method()
    -457        ylim = ax0.get_ylim()
    -458        ax0.fill_betweenx(ylim, x1=retval.value - retval.dvalue, x2=retval.value + retval.dvalue, color='gray', alpha=0.4)
    -459        ax0.set_ylim(ylim)
    -460        ax0.set_ylabel(r'$t^2 \langle E(t) \rangle - 0.3 $')
    -461        xlim = ax0.get_xlim()
    -462
    -463        fit_res = [fit_result[0] + fit_result[1] * xi for xi in x]
    -464        residuals = (np.asarray([o.value for o in y]) - [o.value for o in fit_res]) / np.asarray([o.dvalue for o in y])
    -465        ax1 = plt.subplot(gs[1])
    -466        ax1.plot(x, residuals, 'ko', ls='none', markersize=5)
    -467        ax1.tick_params(direction='out')
    -468        ax1.tick_params(axis="x", bottom=True, top=True, labelbottom=True)
    -469        ax1.axhline(y=0.0, ls='--', color='k')
    -470        ax1.fill_between(xlim, -1.0, 1.0, alpha=0.1, facecolor='k')
    -471        ax1.set_xlim(xlim)
    -472        ax1.set_ylabel('Residuals')
    -473        ax1.set_xlabel(r'$t/a^2$')
    -474
    -475        plt.draw()
    -476    return -fit_result[0] / fit_result[1]
    +363            configlist.append([])
    +364            while True:
    +365                t = fp.read(4)
    +366                if (len(t) < 4):
    +367                    break
    +368                nc = struct.unpack('i', t)[0]
    +369                configlist[-1].append(nc)
    +370
    +371                t = fp.read(8 * tmax * (nn + 1))
    +372                if kwargs.get('plaquette'):
    +373                    if nc % dtr_read == 0:
    +374                        Ysl.append(struct.unpack('d' * tmax * (nn + 1), t))
    +375                t = fp.read(8 * tmax * (nn + 1))
    +376                if not kwargs.get('plaquette'):
    +377                    if nc % dtr_read == 0:
    +378                        Ysl.append(struct.unpack('d' * tmax * (nn + 1), t))
    +379                t = fp.read(8 * tmax * (nn + 1))
    +380
    +381        Ysum.append([])
    +382        for i, item in enumerate(Ysl):
    +383            Ysum[-1].append([np.mean(item[current + xmin:
    +384                             current + tmax - xmin])
    +385                            for current in range(0, len(item), tmax)])
    +386
    +387        diffmeas = configlist[-1][-1] - configlist[-1][-2]
    +388        configlist[-1] = [item // diffmeas for item in configlist[-1]]
    +389        if kwargs.get('assume_thermalization', True) and configlist[-1][0] > 1:
    +390            warnings.warn('Assume thermalization and that the first measurement belongs to the first config.')
    +391            offset = configlist[-1][0] - 1
    +392            configlist[-1] = [item - offset for item in configlist[-1]]
    +393
    +394        if r_start[rep] is None:
    +395            r_start_index.append(0)
    +396        else:
    +397            try:
    +398                r_start_index.append(configlist[-1].index(r_start[rep]))
    +399            except ValueError:
    +400                raise Exception('Config %d not in file with range [%d, %d]' % (
    +401                    r_start[rep], configlist[-1][0], configlist[-1][-1])) from None
    +402
    +403        if r_stop[rep] is None:
    +404            r_stop_index.append(len(configlist[-1]) - 1)
    +405        else:
    +406            try:
    +407                r_stop_index.append(configlist[-1].index(r_stop[rep]))
    +408            except ValueError:
    +409                raise Exception('Config %d not in file with range [%d, %d]' % (
    +410                    r_stop[rep], configlist[-1][0], configlist[-1][-1])) from None
    +411
    +412    if np.any([len(np.unique(np.diff(cl))) != 1 for cl in configlist]):
    +413        raise Exception('Irregular spaced data in input file!', [len(np.unique(np.diff(cl))) for cl in configlist])
    +414    stepsizes = [list(np.unique(np.diff(cl)))[0] for cl in configlist]
    +415    if np.any([step != 1 for step in stepsizes]):
    +416        warnings.warn('Stepsize between configurations is greater than one!' + str(stepsizes), RuntimeWarning)
    +417
    +418    idl = [range(configlist[rep][r_start_index[rep]], configlist[rep][r_stop_index[rep]] + 1, r_step) for rep in range(replica)]
    +419    t2E_dict = {}
    +420    for n in range(nn + 1):
    +421        samples = []
    +422        for nrep, rep in enumerate(Ysum):
    +423            samples.append([])
    +424            for cnfg in rep:
    +425                samples[-1].append(cnfg[n])
    +426            samples[-1] = samples[-1][r_start_index[nrep]:r_stop_index[nrep] + 1][::r_step]
    +427        new_obs = Obs(samples, rep_names, idl=idl)
    +428        t2E_dict[n * dn * eps] = (n * dn * eps) ** 2 * new_obs / (spatial_extent ** 3) - 0.3
    +429
    +430    return fit_t0(t2E_dict, fit_range, plot_fit=kwargs.get('plot_fit'))
     
    @@ -1902,57 +1812,57 @@ Extracted t0
    -
    564def read_qtop(path, prefix, c, dtr_cnfg=1, version="openQCD", **kwargs):
    -565    """Read the topologial charge based on openQCD gradient flow measurements.
    -566
    -567    Parameters
    -568    ----------
    -569    path : str
    -570        path of the measurement files
    -571    prefix : str
    -572        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat.
    -573        Ignored if file names are passed explicitly via keyword files.
    -574    c : double
    -575        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    -576    dtr_cnfg : int
    -577        (optional) parameter that specifies the number of measurements
    -578        between two configs.
    -579        If it is not set, the distance between two measurements
    -580        in the file is assumed to be the distance between two configurations.
    -581    steps : int
    -582        (optional) Distance between two configurations in units of trajectories /
    -583         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    -584    version : str
    -585        Either openQCD or sfqcd, depending on the data.
    -586    L : int
    -587        spatial length of the lattice in L/a.
    -588        HAS to be set if version != sfqcd, since openQCD does not provide
    -589        this in the header
    -590    r_start : list
    -591        list which contains the first config to be read for each replicum.
    -592    r_stop : list
    -593        list which contains the last config to be read for each replicum.
    -594    files : list
    -595        specify the exact files that need to be read
    -596        from path, practical if e.g. only one replicum is needed
    -597    postfix : str
    -598        postfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    -599    names : list
    -600        Alternative labeling for replicas/ensembles.
    -601        Has to have the appropriate length.
    -602    Zeuthen_flow : bool
    -603        (optional) If True, the Zeuthen flow is used for Qtop. Only possible
    -604        for version=='sfqcd' If False, the Wilson flow is used.
    -605    integer_charge : bool
    -606        If True, the charge is rounded towards the nearest integer on each config.
    -607
    -608    Returns
    -609    -------
    -610    result : Obs
    -611        Read topological charge
    -612    """
    -613
    -614    return _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version=version, obspos=0, **kwargs)
    +            
    518def read_qtop(path, prefix, c, dtr_cnfg=1, version="openQCD", **kwargs):
    +519    """Read the topologial charge based on openQCD gradient flow measurements.
    +520
    +521    Parameters
    +522    ----------
    +523    path : str
    +524        path of the measurement files
    +525    prefix : str
    +526        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat.
    +527        Ignored if file names are passed explicitly via keyword files.
    +528    c : double
    +529        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    +530    dtr_cnfg : int
    +531        (optional) parameter that specifies the number of measurements
    +532        between two configs.
    +533        If it is not set, the distance between two measurements
    +534        in the file is assumed to be the distance between two configurations.
    +535    steps : int
    +536        (optional) Distance between two configurations in units of trajectories /
    +537         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    +538    version : str
    +539        Either openQCD or sfqcd, depending on the data.
    +540    L : int
    +541        spatial length of the lattice in L/a.
    +542        HAS to be set if version != sfqcd, since openQCD does not provide
    +543        this in the header
    +544    r_start : list
    +545        list which contains the first config to be read for each replicum.
    +546    r_stop : list
    +547        list which contains the last config to be read for each replicum.
    +548    files : list
    +549        specify the exact files that need to be read
    +550        from path, practical if e.g. only one replicum is needed
    +551    postfix : str
    +552        postfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    +553    names : list
    +554        Alternative labeling for replicas/ensembles.
    +555        Has to have the appropriate length.
    +556    Zeuthen_flow : bool
    +557        (optional) If True, the Zeuthen flow is used for Qtop. Only possible
    +558        for version=='sfqcd' If False, the Wilson flow is used.
    +559    integer_charge : bool
    +560        If True, the charge is rounded towards the nearest integer on each config.
    +561
    +562    Returns
    +563    -------
    +564    result : Obs
    +565        Read topological charge
    +566    """
    +567
    +568    return _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version=version, obspos=0, **kwargs)
     
    @@ -2022,76 +1932,76 @@ Read topological charge
    -
    617def read_gf_coupling(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):
    -618    """Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.
    +            
    571def read_gf_coupling(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):
    +572    """Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.
    +573
    +574    Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.
    +575
    +576    Parameters
    +577    ----------
    +578    path : str
    +579        path of the measurement files
    +580    prefix : str
    +581        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat.
    +582        Ignored if file names are passed explicitly via keyword files.
    +583    c : double
    +584        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    +585    dtr_cnfg : int
    +586        (optional) parameter that specifies the number of measurements
    +587        between two configs.
    +588        If it is not set, the distance between two measurements
    +589        in the file is assumed to be the distance between two configurations.
    +590    steps : int
    +591        (optional) Distance between two configurations in units of trajectories /
    +592         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    +593    r_start : list
    +594        list which contains the first config to be read for each replicum.
    +595    r_stop : list
    +596        list which contains the last config to be read for each replicum.
    +597    files : list
    +598        specify the exact files that need to be read
    +599        from path, practical if e.g. only one replicum is needed
    +600    names : list
    +601        Alternative labeling for replicas/ensembles.
    +602        Has to have the appropriate length.
    +603    postfix : str
    +604        postfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    +605    Zeuthen_flow : bool
    +606        (optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
    +607    """
    +608
    +609    if c != 0.3:
    +610        raise Exception("The required lattice norm is only implemented for c=0.3 at the moment.")
    +611
    +612    plaq = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=6, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs)
    +613    C2x1 = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=7, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs)
    +614    L = plaq.tag["L"]
    +615    T = plaq.tag["T"]
    +616
    +617    if T != L:
    +618        raise Exception("The required lattice norm is only implemented for T=L at the moment.")
     619
    -620    Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.
    -621
    -622    Parameters
    -623    ----------
    -624    path : str
    -625        path of the measurement files
    -626    prefix : str
    -627        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat.
    -628        Ignored if file names are passed explicitly via keyword files.
    -629    c : double
    -630        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    -631    dtr_cnfg : int
    -632        (optional) parameter that specifies the number of measurements
    -633        between two configs.
    -634        If it is not set, the distance between two measurements
    -635        in the file is assumed to be the distance between two configurations.
    -636    steps : int
    -637        (optional) Distance between two configurations in units of trajectories /
    -638         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    -639    r_start : list
    -640        list which contains the first config to be read for each replicum.
    -641    r_stop : list
    -642        list which contains the last config to be read for each replicum.
    -643    files : list
    -644        specify the exact files that need to be read
    -645        from path, practical if e.g. only one replicum is needed
    -646    names : list
    -647        Alternative labeling for replicas/ensembles.
    -648        Has to have the appropriate length.
    -649    postfix : str
    -650        postfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    -651    Zeuthen_flow : bool
    -652        (optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
    -653    """
    -654
    -655    if c != 0.3:
    -656        raise Exception("The required lattice norm is only implemented for c=0.3 at the moment.")
    -657
    -658    plaq = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=6, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs)
    -659    C2x1 = _read_flow_obs(path, prefix, c, dtr_cnfg=dtr_cnfg, version="sfqcd", obspos=7, sum_t=False, Zeuthen_flow=Zeuthen_flow, integer_charge=False, **kwargs)
    -660    L = plaq.tag["L"]
    -661    T = plaq.tag["T"]
    -662
    -663    if T != L:
    -664        raise Exception("The required lattice norm is only implemented for T=L at the moment.")
    -665
    -666    if Zeuthen_flow is not True:
    -667        raise Exception("The required lattice norm is only implemented for the Zeuthen flow at the moment.")
    -668
    -669    t = (c * L) ** 2 / 8
    -670
    -671    normdict = {4: 0.012341170468270,
    -672                6: 0.010162691462430,
    -673                8: 0.009031614807931,
    -674                10: 0.008744966371393,
    -675                12: 0.008650917856809,
    -676                14: 8.611154391267955E-03,
    -677                16: 0.008591758449508,
    -678                20: 0.008575359627103,
    -679                24: 0.008569387847540,
    -680                28: 8.566803713382559E-03,
    -681                32: 0.008565541650006,
    -682                40: 8.564480684962046E-03,
    -683                48: 8.564098025073460E-03,
    -684                64: 8.563853943383087E-03}
    -685
    -686    return t * t * (5 / 3 * plaq - 1 / 12 * C2x1) / normdict[L]
    +620    if Zeuthen_flow is not True:
    +621        raise Exception("The required lattice norm is only implemented for the Zeuthen flow at the moment.")
    +622
    +623    t = (c * L) ** 2 / 8
    +624
    +625    normdict = {4: 0.012341170468270,
    +626                6: 0.010162691462430,
    +627                8: 0.009031614807931,
    +628                10: 0.008744966371393,
    +629                12: 0.008650917856809,
    +630                14: 8.611154391267955E-03,
    +631                16: 0.008591758449508,
    +632                20: 0.008575359627103,
    +633                24: 0.008569387847540,
    +634                28: 8.566803713382559E-03,
    +635                32: 0.008565541650006,
    +636                40: 8.564480684962046E-03,
    +637                48: 8.564098025073460E-03,
    +638                64: 8.563853943383087E-03}
    +639
    +640    return t * t * (5 / 3 * plaq - 1 / 12 * C2x1) / normdict[L]
     
    @@ -2147,30 +2057,30 @@ postfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    -
    961def qtop_projection(qtop, target=0):
    -962    """Returns the projection to the topological charge sector defined by target.
    -963
    -964    Parameters
    -965    ----------
    -966    path : Obs
    -967        Topological charge.
    -968    target : int
    -969        Specifies the topological sector to be reweighted to (default 0)
    -970
    -971    Returns
    -972    -------
    -973    reto : Obs
    -974        projection to the topological charge sector defined by target
    -975    """
    -976    if qtop.reweighted:
    -977        raise Exception('You can not use a reweighted observable for reweighting!')
    -978
    -979    proj_qtop = []
    -980    for n in qtop.deltas:
    -981        proj_qtop.append(np.array([1 if round(qtop.r_values[n] + q) == target else 0 for q in qtop.deltas[n]]))
    -982
    -983    reto = Obs(proj_qtop, qtop.names, idl=[qtop.idl[name] for name in qtop.names])
    -984    return reto
    +            
    915def qtop_projection(qtop, target=0):
    +916    """Returns the projection to the topological charge sector defined by target.
    +917
    +918    Parameters
    +919    ----------
    +920    path : Obs
    +921        Topological charge.
    +922    target : int
    +923        Specifies the topological sector to be reweighted to (default 0)
    +924
    +925    Returns
    +926    -------
    +927    reto : Obs
    +928        projection to the topological charge sector defined by target
    +929    """
    +930    if qtop.reweighted:
    +931        raise Exception('You can not use a reweighted observable for reweighting!')
    +932
    +933    proj_qtop = []
    +934    for n in qtop.deltas:
    +935        proj_qtop.append(np.array([1 if round(qtop.r_values[n] + q) == target else 0 for q in qtop.deltas[n]]))
    +936
    +937    reto = Obs(proj_qtop, qtop.names, idl=[qtop.idl[name] for name in qtop.names])
    +938    return reto
     
    @@ -2206,62 +2116,62 @@ projection to the topological charge sector defined by target
    -
     987def read_qtop_sector(path, prefix, c, target=0, **kwargs):
    - 988    """Constructs reweighting factors to a specified topological sector.
    - 989
    - 990    Parameters
    - 991    ----------
    - 992    path : str
    - 993        path of the measurement files
    - 994    prefix : str
    - 995        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat
    - 996    c : double
    - 997        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L
    - 998    target : int
    - 999        Specifies the topological sector to be reweighted to (default 0)
    -1000    dtr_cnfg : int
    -1001        (optional) parameter that specifies the number of trajectories
    -1002        between two configs.
    -1003        if it is not set, the distance between two measurements
    -1004        in the file is assumed to be the distance between two configurations.
    -1005    steps : int
    -1006        (optional) Distance between two configurations in units of trajectories /
    -1007         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    -1008    version : str
    -1009        version string of the openQCD (sfqcd) version used to create
    -1010        the ensemble. Default is 2.0. May also be set to sfqcd.
    -1011    L : int
    -1012        spatial length of the lattice in L/a.
    -1013        HAS to be set if version != sfqcd, since openQCD does not provide
    -1014        this in the header
    -1015    r_start : list
    -1016        offset of the first ensemble, making it easier to match
    -1017        later on with other Obs
    -1018    r_stop : list
    -1019        last configurations that need to be read (per replicum)
    -1020    files : list
    -1021        specify the exact files that need to be read
    -1022        from path, practical if e.g. only one replicum is needed
    -1023    names : list
    -1024        Alternative labeling for replicas/ensembles.
    -1025        Has to have the appropriate length
    -1026    Zeuthen_flow : bool
    -1027        (optional) If True, the Zeuthen flow is used for Qtop. Only possible
    -1028        for version=='sfqcd' If False, the Wilson flow is used.
    -1029
    -1030    Returns
    -1031    -------
    -1032    reto : Obs
    -1033        projection to the topological charge sector defined by target
    -1034    """
    -1035
    -1036    if not isinstance(target, int):
    -1037        raise Exception("'target' has to be an integer.")
    -1038
    -1039    kwargs['integer_charge'] = True
    -1040    qtop = read_qtop(path, prefix, c, **kwargs)
    -1041
    -1042    return qtop_projection(qtop, target=target)
    +            
    941def read_qtop_sector(path, prefix, c, target=0, **kwargs):
    +942    """Constructs reweighting factors to a specified topological sector.
    +943
    +944    Parameters
    +945    ----------
    +946    path : str
    +947        path of the measurement files
    +948    prefix : str
    +949        prefix of the measurement files, e.g. <prefix>_id0_r0.ms.dat
    +950    c : double
    +951        Smearing radius in units of the lattice extent, c = sqrt(8 t0) / L
    +952    target : int
    +953        Specifies the topological sector to be reweighted to (default 0)
    +954    dtr_cnfg : int
    +955        (optional) parameter that specifies the number of trajectories
    +956        between two configs.
    +957        if it is not set, the distance between two measurements
    +958        in the file is assumed to be the distance between two configurations.
    +959    steps : int
    +960        (optional) Distance between two configurations in units of trajectories /
    +961         cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    +962    version : str
    +963        version string of the openQCD (sfqcd) version used to create
    +964        the ensemble. Default is 2.0. May also be set to sfqcd.
    +965    L : int
    +966        spatial length of the lattice in L/a.
    +967        HAS to be set if version != sfqcd, since openQCD does not provide
    +968        this in the header
    +969    r_start : list
    +970        offset of the first ensemble, making it easier to match
    +971        later on with other Obs
    +972    r_stop : list
    +973        last configurations that need to be read (per replicum)
    +974    files : list
    +975        specify the exact files that need to be read
    +976        from path, practical if e.g. only one replicum is needed
    +977    names : list
    +978        Alternative labeling for replicas/ensembles.
    +979        Has to have the appropriate length
    +980    Zeuthen_flow : bool
    +981        (optional) If True, the Zeuthen flow is used for Qtop. Only possible
    +982        for version=='sfqcd' If False, the Wilson flow is used.
    +983
    +984    Returns
    +985    -------
    +986    reto : Obs
    +987        projection to the topological charge sector defined by target
    +988    """
    +989
    +990    if not isinstance(target, int):
    +991        raise Exception("'target' has to be an integer.")
    +992
    +993    kwargs['integer_charge'] = True
    +994    qtop = read_qtop(path, prefix, c, **kwargs)
    +995
    +996    return qtop_projection(qtop, target=target)
     
    @@ -2330,159 +2240,159 @@ projection to the topological charge sector defined by target
    -
    1045def read_ms5_xsf(path, prefix, qc, corr, sep="r", **kwargs):
    -1046    """
    -1047    Read data from files in the specified directory with the specified prefix and quark combination extension, and return a `Corr` object containing the data.
    -1048
    -1049    Parameters
    -1050    ----------
    -1051    path : str
    -1052        The directory to search for the files in.
    -1053    prefix : str
    -1054        The prefix to match the files against.
    -1055    qc : str
    -1056        The quark combination extension to match the files against.
    -1057    corr : str
    -1058        The correlator to extract data for.
    -1059    sep : str, optional
    -1060        The separator to use when parsing the replika names.
    -1061    **kwargs
    -1062        Additional keyword arguments. The following keyword arguments are recognized:
    -1063
    -1064        - names (List[str]): A list of names to use for the replicas.
    -1065
    -1066    Returns
    -1067    -------
    -1068    Corr
    -1069        A complex valued `Corr` object containing the data read from the files. In case of boudary to bulk correlators.
    -1070    or
    -1071    CObs
    -1072        A complex valued `CObs` object containing the data read from the files. In case of boudary to boundary correlators.
    -1073
    -1074
    -1075    Raises
    -1076    ------
    -1077    FileNotFoundError
    -1078        If no files matching the specified prefix and quark combination extension are found in the specified directory.
    -1079    IOError
    -1080        If there is an error reading a file.
    -1081    struct.error
    -1082        If there is an error unpacking binary data.
    -1083    """
    -1084
    -1085    # found = []
    -1086    files = []
    -1087    names = []
    -1088
    -1089    # test if the input is correct
    -1090    if qc not in ['dd', 'ud', 'du', 'uu']:
    -1091        raise Exception("Unknown quark conbination!")
    -1092
    -1093    if corr not in ["gS", "gP", "gA", "gV", "gVt", "lA", "lV", "lVt", "lT", "lTt", "g1", "l1"]:
    -1094        raise Exception("Unknown correlator!")
    -1095
    -1096    if "files" in kwargs:
    -1097        known_files = kwargs.get("files")
    -1098    else:
    -1099        known_files = []
    -1100    files = _find_files(path, prefix, "ms5_xsf_" + qc, "dat", known_files=known_files)
    +            
     999def read_ms5_xsf(path, prefix, qc, corr, sep="r", **kwargs):
    +1000    """
    +1001    Read data from files in the specified directory with the specified prefix and quark combination extension, and return a `Corr` object containing the data.
    +1002
    +1003    Parameters
    +1004    ----------
    +1005    path : str
    +1006        The directory to search for the files in.
    +1007    prefix : str
    +1008        The prefix to match the files against.
    +1009    qc : str
    +1010        The quark combination extension to match the files against.
    +1011    corr : str
    +1012        The correlator to extract data for.
    +1013    sep : str, optional
    +1014        The separator to use when parsing the replika names.
    +1015    **kwargs
    +1016        Additional keyword arguments. The following keyword arguments are recognized:
    +1017
    +1018        - names (List[str]): A list of names to use for the replicas.
    +1019
    +1020    Returns
    +1021    -------
    +1022    Corr
    +1023        A complex valued `Corr` object containing the data read from the files. In case of boudary to bulk correlators.
    +1024    or
    +1025    CObs
    +1026        A complex valued `CObs` object containing the data read from the files. In case of boudary to boundary correlators.
    +1027
    +1028
    +1029    Raises
    +1030    ------
    +1031    FileNotFoundError
    +1032        If no files matching the specified prefix and quark combination extension are found in the specified directory.
    +1033    IOError
    +1034        If there is an error reading a file.
    +1035    struct.error
    +1036        If there is an error unpacking binary data.
    +1037    """
    +1038
    +1039    # found = []
    +1040    files = []
    +1041    names = []
    +1042
    +1043    # test if the input is correct
    +1044    if qc not in ['dd', 'ud', 'du', 'uu']:
    +1045        raise Exception("Unknown quark conbination!")
    +1046
    +1047    if corr not in ["gS", "gP", "gA", "gV", "gVt", "lA", "lV", "lVt", "lT", "lTt", "g1", "l1"]:
    +1048        raise Exception("Unknown correlator!")
    +1049
    +1050    if "files" in kwargs:
    +1051        known_files = kwargs.get("files")
    +1052    else:
    +1053        known_files = []
    +1054    files = _find_files(path, prefix, "ms5_xsf_" + qc, "dat", known_files=known_files)
    +1055
    +1056    if "names" in kwargs:
    +1057        names = kwargs.get("names")
    +1058    else:
    +1059        for f in files:
    +1060            if not sep == "":
    +1061                se = f.split(".")[0]
    +1062                for s in f.split(".")[1:-2]:
    +1063                    se += "." + s
    +1064                names.append(se.split(sep)[0] + "|r" + se.split(sep)[1])
    +1065            else:
    +1066                names.append(prefix)
    +1067
    +1068    names = sorted(names)
    +1069    files = sorted(files)
    +1070
    +1071    cnfgs = []
    +1072    realsamples = []
    +1073    imagsamples = []
    +1074    repnum = 0
    +1075    for file in files:
    +1076        with open(path + "/" + file, "rb") as fp:
    +1077
    +1078            t = fp.read(8)
    +1079            kappa = struct.unpack('d', t)[0]
    +1080            t = fp.read(8)
    +1081            csw = struct.unpack('d', t)[0]
    +1082            t = fp.read(8)
    +1083            dF = struct.unpack('d', t)[0]
    +1084            t = fp.read(8)
    +1085            zF = struct.unpack('d', t)[0]
    +1086
    +1087            t = fp.read(4)
    +1088            tmax = struct.unpack('i', t)[0]
    +1089            t = fp.read(4)
    +1090            bnd = struct.unpack('i', t)[0]
    +1091
    +1092            placesBI = ["gS", "gP",
    +1093                        "gA", "gV",
    +1094                        "gVt", "lA",
    +1095                        "lV", "lVt",
    +1096                        "lT", "lTt"]
    +1097            placesBB = ["g1", "l1"]
    +1098
    +1099            # the chunks have the following structure:
    +1100            # confignumber, 10x timedependent complex correlators as doubles, 2x timeindependent complex correlators as doubles
     1101
    -1102    if "names" in kwargs:
    -1103        names = kwargs.get("names")
    -1104    else:
    -1105        for f in files:
    -1106            if not sep == "":
    -1107                se = f.split(".")[0]
    -1108                for s in f.split(".")[1:-2]:
    -1109                    se += "." + s
    -1110                names.append(se.split(sep)[0] + "|r" + se.split(sep)[1])
    -1111            else:
    -1112                names.append(prefix)
    -1113
    -1114    names = sorted(names)
    -1115    files = sorted(files)
    -1116
    -1117    cnfgs = []
    -1118    realsamples = []
    -1119    imagsamples = []
    -1120    repnum = 0
    -1121    for file in files:
    -1122        with open(path + "/" + file, "rb") as fp:
    +1102            chunksize = 4 + (8 * 2 * tmax * 10) + (8 * 2 * 2)
    +1103            packstr = '=i' + ('d' * 2 * tmax * 10) + ('d' * 2 * 2)
    +1104            cnfgs.append([])
    +1105            realsamples.append([])
    +1106            imagsamples.append([])
    +1107            for t in range(tmax):
    +1108                realsamples[repnum].append([])
    +1109                imagsamples[repnum].append([])
    +1110
    +1111            while True:
    +1112                cnfgt = fp.read(chunksize)
    +1113                if not cnfgt:
    +1114                    break
    +1115                asascii = struct.unpack(packstr, cnfgt)
    +1116                cnfg = asascii[0]
    +1117                cnfgs[repnum].append(cnfg)
    +1118
    +1119                if corr not in placesBB:
    +1120                    tmpcorr = asascii[1 + 2 * tmax * placesBI.index(corr):1 + 2 * tmax * placesBI.index(corr) + 2 * tmax]
    +1121                else:
    +1122                    tmpcorr = asascii[1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr):1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr) + 2]
     1123
    -1124            t = fp.read(8)
    -1125            kappa = struct.unpack('d', t)[0]
    -1126            t = fp.read(8)
    -1127            csw = struct.unpack('d', t)[0]
    -1128            t = fp.read(8)
    -1129            dF = struct.unpack('d', t)[0]
    -1130            t = fp.read(8)
    -1131            zF = struct.unpack('d', t)[0]
    +1124                corrres = [[], []]
    +1125                for i in range(len(tmpcorr)):
    +1126                    corrres[i % 2].append(tmpcorr[i])
    +1127                for t in range(int(len(tmpcorr) / 2)):
    +1128                    realsamples[repnum][t].append(corrres[0][t])
    +1129                for t in range(int(len(tmpcorr) / 2)):
    +1130                    imagsamples[repnum][t].append(corrres[1][t])
    +1131        repnum += 1
     1132
    -1133            t = fp.read(4)
    -1134            tmax = struct.unpack('i', t)[0]
    -1135            t = fp.read(4)
    -1136            bnd = struct.unpack('i', t)[0]
    -1137
    -1138            placesBI = ["gS", "gP",
    -1139                        "gA", "gV",
    -1140                        "gVt", "lA",
    -1141                        "lV", "lVt",
    -1142                        "lT", "lTt"]
    -1143            placesBB = ["g1", "l1"]
    -1144
    -1145            # the chunks have the following structure:
    -1146            # confignumber, 10x timedependent complex correlators as doubles, 2x timeindependent complex correlators as doubles
    +1133    s = "Read correlator " + corr + " from " + str(repnum) + " replika with " + str(len(realsamples[0][t]))
    +1134    for rep in range(1, repnum):
    +1135        s += ", " + str(len(realsamples[rep][t]))
    +1136    s += " samples"
    +1137    print(s)
    +1138    print("Asserted run parameters:\n T:", tmax, "kappa:", kappa, "csw:", csw, "dF:", dF, "zF:", zF, "bnd:", bnd)
    +1139
    +1140    # we have the data now... but we need to re format the whole thing and put it into Corr objects.
    +1141
    +1142    compObs = []
    +1143
    +1144    for t in range(int(len(tmpcorr) / 2)):
    +1145        compObs.append(CObs(Obs([realsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs),
    +1146                            Obs([imagsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs)))
     1147
    -1148            chunksize = 4 + (8 * 2 * tmax * 10) + (8 * 2 * 2)
    -1149            packstr = '=i' + ('d' * 2 * tmax * 10) + ('d' * 2 * 2)
    -1150            cnfgs.append([])
    -1151            realsamples.append([])
    -1152            imagsamples.append([])
    -1153            for t in range(tmax):
    -1154                realsamples[repnum].append([])
    -1155                imagsamples[repnum].append([])
    -1156
    -1157            while True:
    -1158                cnfgt = fp.read(chunksize)
    -1159                if not cnfgt:
    -1160                    break
    -1161                asascii = struct.unpack(packstr, cnfgt)
    -1162                cnfg = asascii[0]
    -1163                cnfgs[repnum].append(cnfg)
    -1164
    -1165                if corr not in placesBB:
    -1166                    tmpcorr = asascii[1 + 2 * tmax * placesBI.index(corr):1 + 2 * tmax * placesBI.index(corr) + 2 * tmax]
    -1167                else:
    -1168                    tmpcorr = asascii[1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr):1 + 2 * tmax * len(placesBI) + 2 * placesBB.index(corr) + 2]
    -1169
    -1170                corrres = [[], []]
    -1171                for i in range(len(tmpcorr)):
    -1172                    corrres[i % 2].append(tmpcorr[i])
    -1173                for t in range(int(len(tmpcorr) / 2)):
    -1174                    realsamples[repnum][t].append(corrres[0][t])
    -1175                for t in range(int(len(tmpcorr) / 2)):
    -1176                    imagsamples[repnum][t].append(corrres[1][t])
    -1177        repnum += 1
    -1178
    -1179    s = "Read correlator " + corr + " from " + str(repnum) + " replika with " + str(len(realsamples[0][t]))
    -1180    for rep in range(1, repnum):
    -1181        s += ", " + str(len(realsamples[rep][t]))
    -1182    s += " samples"
    -1183    print(s)
    -1184    print("Asserted run parameters:\n T:", tmax, "kappa:", kappa, "csw:", csw, "dF:", dF, "zF:", zF, "bnd:", bnd)
    -1185
    -1186    # we have the data now... but we need to re format the whole thing and put it into Corr objects.
    -1187
    -1188    compObs = []
    -1189
    -1190    for t in range(int(len(tmpcorr) / 2)):
    -1191        compObs.append(CObs(Obs([realsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs),
    -1192                            Obs([imagsamples[rep][t] for rep in range(repnum)], names=names, idl=cnfgs)))
    -1193
    -1194    if len(compObs) == 1:
    -1195        return compObs[0]
    -1196    else:
    -1197        return Corr(compObs)
    +1148    if len(compObs) == 1:
    +1149        return compObs[0]
    +1150    else:
    +1151        return Corr(compObs)
     
    diff --git a/docs/pyerrors/input/pandas.html b/docs/pyerrors/input/pandas.html index 14b7940b..345f182c 100644 --- a/docs/pyerrors/input/pandas.html +++ b/docs/pyerrors/input/pandas.html @@ -3,7 +3,7 @@ - + pyerrors.input.pandas API documentation diff --git a/docs/pyerrors/input/sfcf.html b/docs/pyerrors/input/sfcf.html index 399fe256..8479d85a 100644 --- a/docs/pyerrors/input/sfcf.html +++ b/docs/pyerrors/input/sfcf.html @@ -3,7 +3,7 @@ - + pyerrors.input.sfcf API documentation diff --git a/docs/pyerrors/input/utils.html b/docs/pyerrors/input/utils.html index 0c79029c..35d788be 100644 --- a/docs/pyerrors/input/utils.html +++ b/docs/pyerrors/input/utils.html @@ -3,7 +3,7 @@ - + pyerrors.input.utils API documentation diff --git a/docs/pyerrors/linalg.html b/docs/pyerrors/linalg.html index 90c4b97e..ace6383d 100644 --- a/docs/pyerrors/linalg.html +++ b/docs/pyerrors/linalg.html @@ -3,7 +3,7 @@ - + pyerrors.linalg API documentation diff --git a/docs/pyerrors/misc.html b/docs/pyerrors/misc.html index 363a6d26..59a399e5 100644 --- a/docs/pyerrors/misc.html +++ b/docs/pyerrors/misc.html @@ -3,7 +3,7 @@ - + pyerrors.misc API documentation diff --git a/docs/pyerrors/mpm.html b/docs/pyerrors/mpm.html index 5c3b6efd..40eabfd8 100644 --- a/docs/pyerrors/mpm.html +++ b/docs/pyerrors/mpm.html @@ -3,7 +3,7 @@ - + pyerrors.mpm API documentation diff --git a/docs/pyerrors/obs.html b/docs/pyerrors/obs.html index 1d790a77..af2eb985 100644 --- a/docs/pyerrors/obs.html +++ b/docs/pyerrors/obs.html @@ -3,7 +3,7 @@ - + pyerrors.obs API documentation diff --git a/docs/pyerrors/roots.html b/docs/pyerrors/roots.html index c45c2525..5836a34c 100644 --- a/docs/pyerrors/roots.html +++ b/docs/pyerrors/roots.html @@ -3,7 +3,7 @@ - + pyerrors.roots API documentation diff --git a/docs/pyerrors/version.html b/docs/pyerrors/version.html index 24b90e43..fd00dbdd 100644 --- a/docs/pyerrors/version.html +++ b/docs/pyerrors/version.html @@ -3,7 +3,7 @@ - + pyerrors.version API documentation diff --git a/docs/search.js b/docs/search.js index ddd5b65b..c67e8db8 100644 --- a/docs/search.js +++ b/docs/search.js @@ -1,6 +1,6 @@ window.pdocSearch = (function(){ /** elasticlunr - http://weixsong.github.io * Copyright (C) 2017 Oliver Nightingale * Copyright (C) 2017 Wei Song * MIT Licensed */!function(){function e(e){if(null===e||"object"!=typeof e)return e;var t=e.constructor();for(var n in e)e.hasOwnProperty(n)&&(t[n]=e[n]);return t}var t=function(e){var n=new t.Index;return n.pipeline.add(t.trimmer,t.stopWordFilter,t.stemmer),e&&e.call(n,n),n};t.version="0.9.5",lunr=t,t.utils={},t.utils.warn=function(e){return function(t){e.console&&console.warn&&console.warn(t)}}(this),t.utils.toString=function(e){return void 0===e||null===e?"":e.toString()},t.EventEmitter=function(){this.events={}},t.EventEmitter.prototype.addListener=function(){var e=Array.prototype.slice.call(arguments),t=e.pop(),n=e;if("function"!=typeof t)throw new TypeError("last argument must be a function");n.forEach(function(e){this.hasHandler(e)||(this.events[e]=[]),this.events[e].push(t)},this)},t.EventEmitter.prototype.removeListener=function(e,t){if(this.hasHandler(e)){var n=this.events[e].indexOf(t);-1!==n&&(this.events[e].splice(n,1),0==this.events[e].length&&delete this.events[e])}},t.EventEmitter.prototype.emit=function(e){if(this.hasHandler(e)){var t=Array.prototype.slice.call(arguments,1);this.events[e].forEach(function(e){e.apply(void 0,t)},this)}},t.EventEmitter.prototype.hasHandler=function(e){return e in this.events},t.tokenizer=function(e){if(!arguments.length||null===e||void 0===e)return[];if(Array.isArray(e)){var n=e.filter(function(e){return null===e||void 0===e?!1:!0});n=n.map(function(e){return t.utils.toString(e).toLowerCase()});var i=[];return n.forEach(function(e){var n=e.split(t.tokenizer.seperator);i=i.concat(n)},this),i}return e.toString().trim().toLowerCase().split(t.tokenizer.seperator)},t.tokenizer.defaultSeperator=/[\s\-]+/,t.tokenizer.seperator=t.tokenizer.defaultSeperator,t.tokenizer.setSeperator=function(e){null!==e&&void 0!==e&&"object"==typeof e&&(t.tokenizer.seperator=e)},t.tokenizer.resetSeperator=function(){t.tokenizer.seperator=t.tokenizer.defaultSeperator},t.tokenizer.getSeperator=function(){return t.tokenizer.seperator},t.Pipeline=function(){this._queue=[]},t.Pipeline.registeredFunctions={},t.Pipeline.registerFunction=function(e,n){n in t.Pipeline.registeredFunctions&&t.utils.warn("Overwriting existing registered function: "+n),e.label=n,t.Pipeline.registeredFunctions[n]=e},t.Pipeline.getRegisteredFunction=function(e){return e in t.Pipeline.registeredFunctions!=!0?null:t.Pipeline.registeredFunctions[e]},t.Pipeline.warnIfFunctionNotRegistered=function(e){var n=e.label&&e.label in this.registeredFunctions;n||t.utils.warn("Function is not registered with pipeline. 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this.config},t.Configuration.prototype.reset=function(){this.config={}},lunr.SortedSet=function(){this.length=0,this.elements=[]},lunr.SortedSet.load=function(e){var t=new this;return t.elements=e,t.length=e.length,t},lunr.SortedSet.prototype.add=function(){var e,t;for(e=0;e1;){if(r===e)return o;e>r&&(t=o),r>e&&(n=o),i=n-t,o=t+Math.floor(i/2),r=this.elements[o]}return r===e?o:-1},lunr.SortedSet.prototype.locationFor=function(e){for(var t=0,n=this.elements.length,i=n-t,o=t+Math.floor(i/2),r=this.elements[o];i>1;)e>r&&(t=o),r>e&&(n=o),i=n-t,o=t+Math.floor(i/2),r=this.elements[o];return r>e?o:e>r?o+1:void 0},lunr.SortedSet.prototype.intersect=function(e){for(var t=new lunr.SortedSet,n=0,i=0,o=this.length,r=e.length,s=this.elements,u=e.elements;;){if(n>o-1||i>r-1)break;s[n]!==u[i]?s[n]u[i]&&i++:(t.add(s[n]),n++,i++)}return t},lunr.SortedSet.prototype.clone=function(){var e=new lunr.SortedSet;return e.elements=this.toArray(),e.length=e.elements.length,e},lunr.SortedSet.prototype.union=function(e){var t,n,i;this.length>=e.length?(t=this,n=e):(t=e,n=this),i=t.clone();for(var o=0,r=n.toArray();oWhat is pyerrors?\n\n

    pyerrors is a python package for error computation and propagation of Markov chain Monte Carlo data.\nIt is based on the gamma method arXiv:hep-lat/0306017. Some of its features are:

    \n\n
      \n
    • automatic differentiation for exact linear error propagation as suggested in arXiv:1809.01289 (partly based on the autograd package).
    • \n
    • treatment of slow modes in the simulation as suggested in arXiv:1009.5228.
    • \n
    • coherent error propagation for data from different Markov chains.
    • \n
    • non-linear fits with x- and y-errors and exact linear error propagation based on automatic differentiation as introduced in arXiv:1809.01289.
    • \n
    • real and complex matrix operations and their error propagation based on automatic differentiation (Matrix inverse, Cholesky decomposition, calculation of eigenvalues and eigenvectors, singular value decomposition...).
    • \n
    \n\n

    More detailed examples can found in the GitHub repository \"badge\".

    \n\n

    If you use pyerrors for research that leads to a publication please consider citing:

    \n\n
      \n
    • Fabian Joswig, Simon Kuberski, Justus T. Kuhlmann, Jan Neuendorf, pyerrors: a python framework for error analysis of Monte Carlo data. [arXiv:2209.14371 [hep-lat]].
    • \n
    • Ulli Wolff, Monte Carlo errors with less errors. Comput.Phys.Commun. 156 (2004) 143-153, Comput.Phys.Commun. 176 (2007) 383 (erratum).
    • \n
    • Alberto Ramos, Automatic differentiation for error analysis of Monte Carlo data. Comput.Phys.Commun. 238 (2019) 19-35.
    • \n
    \n\n

    and

    \n\n
      \n
    • Stefan Schaefer, Rainer Sommer, Francesco Virotta, Critical slowing down and error analysis in lattice QCD simulations. Nucl.Phys.B 845 (2011) 93-119.
    • \n
    \n\n

    where applicable.

    \n\n

    There exist similar publicly available implementations of gamma method error analysis suites in Fortran, Julia and Python.

    \n\n

    Installation

    \n\n

    Install the most recent release using pip and pypi:

    \n\n
    \n
    pip install pyerrors     # Fresh install\npip install -U pyerrors  # Update\n
    \n
    \n\n

    Install the most recent release using conda and conda-forge:

    \n\n
    \n
    conda install -c conda-forge pyerrors  # Fresh install\nconda update -c conda-forge pyerrors   # Update\n
    \n
    \n\n

    Install the current develop version:

    \n\n
    \n
    pip install git+https://github.com/fjosw/pyerrors.git@develop\n
    \n
    \n\n

    Basic example

    \n\n
    \n
    import numpy as np\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name']) # Initialize an Obs object\nmy_new_obs = 2 * np.log(my_obs) / my_obs ** 2 # Construct derived Obs object\nmy_new_obs.gamma_method()                     # Estimate the statistical error\nprint(my_new_obs)                             # Print the result to stdout\n> 0.31498(72)\n
    \n
    \n\n

    The Obs class

    \n\n

    pyerrors introduces a new datatype, Obs, which simplifies error propagation and estimation for auto- and cross-correlated data.\nAn Obs object can be initialized with two arguments, the first is a list containing the samples for an observable from a Monte Carlo chain.\nThe samples can either be provided as python list or as numpy array.\nThe second argument is a list containing the names of the respective Monte Carlo chains as strings. These strings uniquely identify a Monte Carlo chain/ensemble. It is crucial for the correct error propagation that observations from the same Monte Carlo history are labeled with the same name. See Multiple ensembles/replica for details.

    \n\n
    \n
    import pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name'])\n
    \n
    \n\n

    Error propagation

    \n\n

    When performing mathematical operations on Obs objects the correct error propagation is intrinsically taken care of using a first order Taylor expansion\n$$\\delta_f^i=\\sum_\\alpha \\bar{f}_\\alpha \\delta_\\alpha^i\\,,\\quad \\delta_\\alpha^i=a_\\alpha^i-\\bar{a}_\\alpha\\,,$$\nas introduced in arXiv:hep-lat/0306017.\nThe required derivatives $\\bar{f}_\\alpha$ are evaluated up to machine precision via automatic differentiation as suggested in arXiv:1809.01289.

    \n\n

    The Obs class is designed such that mathematical numpy functions can be used on Obs just as for regular floats.

    \n\n
    \n
    import numpy as np\nimport pyerrors as pe\n\nmy_obs1 = pe.Obs([samples1], ['ensemble_name'])\nmy_obs2 = pe.Obs([samples2], ['ensemble_name'])\n\nmy_sum = my_obs1 + my_obs2\n\nmy_m_eff = np.log(my_obs1 / my_obs2)\n\niamzero = my_m_eff - my_m_eff\n# Check that value and fluctuations are zero within machine precision\nprint(iamzero == 0.0)\n> True\n
    \n
    \n\n

    Error estimation

    \n\n

    The error estimation within pyerrors is based on the gamma method introduced in arXiv:hep-lat/0306017.\nAfter having arrived at the derived quantity of interest the gamma_method can be called as detailed in the following example.

    \n\n
    \n
    my_sum.gamma_method()\nprint(my_sum)\n> 1.70(57)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 5.72046658e-01 +/- 7.56746598e-02 (33.650%)\n>  t_int         2.71422900e+00 +/- 6.40320983e-01 S = 2.00\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    We use the following definition of the integrated autocorrelation time established in Madras & Sokal 1988\n$$\\tau_\\mathrm{int}=\\frac{1}{2}+\\sum_{t=1}^{W}\\rho(t)\\geq \\frac{1}{2}\\,.$$\nThe window $W$ is determined via the automatic windowing procedure described in arXiv:hep-lat/0306017.\nThe standard value for the parameter $S$ of this automatic windowing procedure is $S=2$. Other values for $S$ can be passed to the gamma_method as parameter.

    \n\n
    \n
    my_sum.gamma_method(S=3.0)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 6.30675201e-01 +/- 1.04585650e-01 (37.099%)\n>  t_int         3.29909703e+00 +/- 9.77310102e-01 S = 3.00\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    The integrated autocorrelation time $\\tau_\\mathrm{int}$ and the autocorrelation function $\\rho(W)$ can be monitored via the methods pyerrors.obs.Obs.plot_tauint and pyerrors.obs.Obs.plot_rho.

    \n\n

    If the parameter $S$ is set to zero it is assumed that the dataset does not exhibit any autocorrelation and the window size is chosen to be zero.\nIn this case the error estimate is identical to the sample standard error.

    \n\n

    Exponential tails

    \n\n

    Slow modes in the Monte Carlo history can be accounted for by attaching an exponential tail to the autocorrelation function $\\rho$ as suggested in arXiv:1009.5228. The longest autocorrelation time in the history, $\\tau_\\mathrm{exp}$, can be passed to the gamma_method as parameter. In this case the automatic windowing procedure is vacated and the parameter $S$ does not affect the error estimate.

    \n\n
    \n
    my_sum.gamma_method(tau_exp=7.2)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 6.28097762e-01 +/- 5.79077524e-02 (36.947%)\n>  t_int         3.27218667e+00 +/- 7.99583654e-01 tau_exp = 7.20,  N_sigma = 1\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    For the full API see pyerrors.obs.Obs.gamma_method.

    \n\n

    Multiple ensembles/replica

    \n\n

    Error propagation for multiple ensembles (Markov chains with different simulation parameters) is handled automatically. Ensembles are uniquely identified by their name.

    \n\n
    \n
    obs1 = pe.Obs([samples1], ['ensemble1'])\nobs2 = pe.Obs([samples2], ['ensemble2'])\n\nmy_sum = obs1 + obs2\nmy_sum.details()\n> Result   2.00697958e+00\n> 1500 samples in 2 ensembles:\n>   \u00b7 Ensemble 'ensemble1' : 1000 configurations (from 1 to 1000)\n>   \u00b7 Ensemble 'ensemble2' : 500 configurations (from 1 to 500)\n
    \n
    \n\n

    Observables from the same Monte Carlo chain have to be initialized with the same name for correct error propagation. If different names were used in this case the data would be treated as statistically independent resulting in loss of relevant information and a potential over or under estimate of the statistical error.

    \n\n

    pyerrors identifies multiple replica (independent Markov chains with identical simulation parameters) by the vertical bar | in the name of the data set.

    \n\n
    \n
    obs1 = pe.Obs([samples1], ['ensemble1|r01'])\nobs2 = pe.Obs([samples2], ['ensemble1|r02'])\n\n> my_sum = obs1 + obs2\n> my_sum.details()\n> Result   2.00697958e+00\n> 1500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1'\n>     \u00b7 Replicum 'r01' : 1000 configurations (from 1 to 1000)\n>     \u00b7 Replicum 'r02' : 500 configurations (from 1 to 500)\n
    \n
    \n\n

    Error estimation for multiple ensembles

    \n\n

    In order to keep track of different error analysis parameters for different ensembles one can make use of global dictionaries as detailed in the following example.

    \n\n
    \n
    pe.Obs.S_dict['ensemble1'] = 2.5\npe.Obs.tau_exp_dict['ensemble2'] = 8.0\npe.Obs.tau_exp_dict['ensemble3'] = 2.0\n
    \n
    \n\n

    In case the gamma_method is called without any parameters it will use the values specified in the dictionaries for the respective ensembles.\nPassing arguments to the gamma_method still dominates over the dictionaries.

    \n\n

    Irregular Monte Carlo chains

    \n\n

    Obs objects defined on irregular Monte Carlo chains can be initialized with the parameter idl.

    \n\n
    \n
    # Observable defined on configurations 20 to 519\nobs1 = pe.Obs([samples1], ['ensemble1'], idl=[range(20, 520)])\nobs1.details()\n> Result         9.98319881e-01\n> 500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 500 configurations (from 20 to 519)\n\n# Observable defined on every second configuration between 5 and 1003\nobs2 = pe.Obs([samples2], ['ensemble1'], idl=[range(5, 1005, 2)])\nobs2.details()\n> Result         9.99100712e-01\n> 500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 500 configurations (from 5 to 1003 in steps of 2)\n\n# Observable defined on configurations 2, 9, 28, 29 and 501\nobs3 = pe.Obs([samples3], ['ensemble1'], idl=[[2, 9, 28, 29, 501]])\nobs3.details()\n> Result         1.01718064e+00\n> 5 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 5 configurations (irregular range)\n
    \n
    \n\n

    Obs objects defined on regular and irregular histories of the same ensemble can be combined with each other and the correct error propagation and estimation is automatically taken care of.

    \n\n

    Warning: Irregular Monte Carlo chains can result in odd patterns in the autocorrelation functions.\nMake sure to check the autocorrelation time with e.g. pyerrors.obs.Obs.plot_rho or pyerrors.obs.Obs.plot_tauint.

    \n\n

    For the full API see pyerrors.obs.Obs.

    \n\n

    Correlators

    \n\n

    When one is not interested in single observables but correlation functions, pyerrors offers the Corr class which simplifies the corresponding error propagation and provides the user with a set of standard methods. In order to initialize a Corr objects one needs to arrange the data as a list of Obs

    \n\n
    \n
    my_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3])\nprint(my_corr)\n> x0/a  Corr(x0/a)\n> ------------------\n> 0      0.7957(80)\n> 1      0.5156(51)\n> 2      0.3227(33)\n> 3      0.2041(21)\n
    \n
    \n\n

    In case the correlation functions are not defined on the outermost timeslices, for example because of fixed boundary conditions, a padding can be introduced.

    \n\n
    \n
    my_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3], padding=[1, 1])\nprint(my_corr)\n> x0/a  Corr(x0/a)\n> ------------------\n> 0\n> 1      0.7957(80)\n> 2      0.5156(51)\n> 3      0.3227(33)\n> 4      0.2041(21)\n> 5\n
    \n
    \n\n

    The individual entries of a correlator can be accessed via slicing

    \n\n
    \n
    print(my_corr[3])\n> 0.3227(33)\n
    \n
    \n\n

    Error propagation with the Corr class works very similar to Obs objects. Mathematical operations are overloaded and Corr objects can be computed together with other Corr objects, Obs objects or real numbers and integers.

    \n\n
    \n
    my_new_corr = 0.3 * my_corr[2] * my_corr * my_corr + 12 / my_corr\n
    \n
    \n\n

    pyerrors provides the user with a set of regularly used methods for the manipulation of correlator objects:

    \n\n
      \n
    • Corr.gamma_method applies the gamma method to all entries of the correlator.
    • \n
    • Corr.m_eff to construct effective masses. Various variants for periodic and fixed temporal boundary conditions are available.
    • \n
    • Corr.deriv returns the first derivative of the correlator as Corr. Different discretizations of the numerical derivative are available.
    • \n
    • Corr.second_deriv returns the second derivative of the correlator as Corr. Different discretizations of the numerical derivative are available.
    • \n
    • Corr.symmetric symmetrizes parity even correlations functions, assuming periodic boundary conditions.
    • \n
    • Corr.anti_symmetric anti-symmetrizes parity odd correlations functions, assuming periodic boundary conditions.
    • \n
    • Corr.T_symmetry averages a correlator with its time symmetry partner, assuming fixed boundary conditions.
    • \n
    • Corr.plateau extracts a plateau value from the correlator in a given range.
    • \n
    • Corr.roll periodically shifts the correlator.
    • \n
    • Corr.reverse reverses the time ordering of the correlator.
    • \n
    • Corr.correlate constructs a disconnected correlation function from the correlator and another Corr or Obs object.
    • \n
    • Corr.reweight reweights the correlator.
    • \n
    \n\n

    pyerrors can also handle matrices of correlation functions and extract energy states from these matrices via a generalized eigenvalue problem (see pyerrors.correlators.Corr.GEVP).

    \n\n

    For the full API see pyerrors.correlators.Corr.

    \n\n

    Complex valued observables

    \n\n

    pyerrors can handle complex valued observables via the class pyerrors.obs.CObs.\nCObs are initialized with a real and an imaginary part which both can be Obs valued.

    \n\n
    \n
    my_real_part = pe.Obs([samples1], ['ensemble1'])\nmy_imag_part = pe.Obs([samples2], ['ensemble1'])\n\nmy_cobs = pe.CObs(my_real_part, my_imag_part)\nmy_cobs.gamma_method()\nprint(my_cobs)\n> (0.9959(91)+0.659(28)j)\n
    \n
    \n\n

    Elementary mathematical operations are overloaded and samples are properly propagated as for the Obs class.

    \n\n
    \n
    my_derived_cobs = (my_cobs + my_cobs.conjugate()) / np.abs(my_cobs)\nmy_derived_cobs.gamma_method()\nprint(my_derived_cobs)\n> (1.668(23)+0.0j)\n
    \n
    \n\n

    The Covobs class

    \n\n

    In many projects, auxiliary data that is not based on Monte Carlo chains enters. Examples are experimentally determined mesons masses which are used to set the scale or renormalization constants. These numbers come with an error that has to be propagated through the analysis. The Covobs class allows to define such quantities in pyerrors. Furthermore, external input might consist of correlated quantities. An example are the parameters of an interpolation formula, which are defined via mean values and a covariance matrix between all parameters. The contribution of the interpolation formula to the error of a derived quantity therefore might depend on the complete covariance matrix.

    \n\n

    This concept is built into the definition of Covobs. In pyerrors, external input is defined by $M$ mean values, a $M\\times M$ covariance matrix, where $M=1$ is permissible, and a name that uniquely identifies the covariance matrix. Below, we define the pion mass, based on its mean value and error, 134.9768(5). Note, that the square of the error enters cov_Obs, since the second argument of this function is the covariance matrix of the Covobs.

    \n\n
    \n
    import pyerrors.obs as pe\n\nmpi = pe.cov_Obs(134.9768, 0.0005**2, 'pi^0 mass')\nmpi.gamma_method()\nmpi.details()\n> Result         1.34976800e+02 +/- 5.00000000e-04 +/- 0.00000000e+00 (0.000%)\n>  pi^0 mass     5.00000000e-04\n> 0 samples in 1 ensemble:\n>   \u00b7 Covobs   'pi^0 mass'\n
    \n
    \n\n

    The resulting object mpi is an Obs that contains a Covobs. In the following, it may be handled as any other Obs. The contribution of the covariance matrix to the error of an Obs is determined from the $M \\times M$ covariance matrix $\\Sigma$ and the gradient of the Obs with respect to the external quantities, which is the $1\\times M$ Jacobian matrix $J$, via\n$$s = \\sqrt{J^T \\Sigma J}\\,,$$\nwhere the Jacobian is computed for each derived quantity via automatic differentiation.

    \n\n

    Correlated auxiliary data is defined similarly to above, e.g., via

    \n\n
    \n
    RAP = pe.cov_Obs([16.7457, -19.0475], [[3.49591, -6.07560], [-6.07560, 10.5834]], 'R_AP, 1906.03445, (5.3a)')\nprint(RAP)\n> [Obs[16.7(1.9)], Obs[-19.0(3.3)]]\n
    \n
    \n\n

    where RAP now is a list of two Obs that contains the two correlated parameters.

    \n\n

    Since the gradient of a derived observable with respect to an external covariance matrix is propagated through the entire analysis, the Covobs class allows to quote the derivative of a result with respect to the external quantities. If these derivatives are published together with the result, small shifts in the definition of external quantities, e.g., the definition of the physical point, can be performed a posteriori based on the published information. This may help to compare results of different groups. The gradient of an Obs o with respect to a covariance matrix with the identifying string k may be accessed via

    \n\n
    \n
    o.covobs[k].grad\n
    \n
    \n\n

    Error propagation in iterative algorithms

    \n\n

    pyerrors supports exact linear error propagation for iterative algorithms like various variants of non-linear least squares fits or root finding. The derivatives required for the error propagation are calculated as described in arXiv:1809.01289.

    \n\n

    Least squares fits

    \n\n

    Standard non-linear least square fits with errors on the dependent but not the independent variables can be performed with pyerrors.fits.least_squares. As default solver the Levenberg-Marquardt algorithm implemented in scipy is used.

    \n\n

    Fit functions have to be of the following form

    \n\n
    \n
    import autograd.numpy as anp\n\ndef func(a, x):\n    return a[1] * anp.exp(-a[0] * x)\n
    \n
    \n\n

    It is important that numerical functions refer to autograd.numpy instead of numpy for the automatic differentiation in iterative algorithms to work properly.

    \n\n

    Fits can then be performed via

    \n\n
    \n
    fit_result = pe.fits.least_squares(x, y, func)\nprint("\\n", fit_result)\n> Fit with 2 parameters\n> Method: Levenberg-Marquardt\n> `ftol` termination condition is satisfied.\n> chisquare/d.o.f.: 0.9593035785160936\n\n>  Goodness of fit:\n> \u03c7\u00b2/d.o.f. = 0.959304\n> p-value   = 0.5673\n> Fit parameters:\n> 0      0.0548(28)\n> 1      1.933(64)\n
    \n
    \n\n

    where x is a list or numpy.array of floats and y is a list or numpy.array of Obs.

    \n\n

    Data stored in Corr objects can be fitted directly using the Corr.fit method.

    \n\n
    \n
    my_corr = pe.Corr(y)\nfit_result = my_corr.fit(func, fitrange=[12, 25])\n
    \n
    \n\n

    this can simplify working with absolute fit ranges and takes care of gaps in the data automatically.

    \n\n

    For fit functions with multiple independent variables the fit function can be of the form

    \n\n
    \n
    def func(a, x):\n    (x1, x2) = x\n    return a[0] * x1 ** 2 + a[1] * x2\n
    \n
    \n\n

    pyerrors also supports correlated fits which can be triggered via the parameter correlated_fit=True.\nDetails about how the required covariance matrix is estimated can be found in pyerrors.obs.covariance.

    \n\n

    Direct visualizations of the performed fits can be triggered via resplot=True or qqplot=True. For all available options see pyerrors.fits.least_squares.

    \n\n

    Total least squares fits

    \n\n

    pyerrors can also fit data with errors on both the dependent and independent variables using the total least squares method also referred to orthogonal distance regression as implemented in scipy, see pyerrors.fits.least_squares. The syntax is identical to the standard least squares case, the only difference being that x also has to be a list or numpy.array of Obs.

    \n\n

    For the full API see pyerrors.fits for fits and pyerrors.roots for finding roots of functions.

    \n\n

    Matrix operations

    \n\n

    pyerrors provides wrappers for Obs- and CObs-valued matrix operations based on numpy.linalg. The supported functions include:

    \n\n
      \n
    • inv for the matrix inverse.
    • \n
    • cholseky for the Cholesky decomposition.
    • \n
    • det for the matrix determinant.
    • \n
    • eigh for eigenvalues and eigenvectors of hermitean matrices.
    • \n
    • eig for eigenvalues of general matrices.
    • \n
    • pinv for the Moore-Penrose pseudoinverse.
    • \n
    • svd for the singular-value-decomposition.
    • \n
    \n\n

    For the full API see pyerrors.linalg.

    \n\n

    Export data

    \n\n

    \n\n

    The preferred exported file format within pyerrors is json.gz. Files written to this format are valid JSON files that have been compressed using gzip. The structure of the content is inspired by the dobs format of the ALPHA collaboration. The aim of the format is to facilitate the storage of data in a self-contained way such that, even years after the creation of the file, it is possible to extract all necessary information:

    \n\n
      \n
    • What observables are stored? Possibly: How exactly are they defined.
    • \n
    • How does each single ensemble or external quantity contribute to the error of the observable?
    • \n
    • Who did write the file when and on which machine?
    • \n
    \n\n

    This can be achieved by storing all information in one single file. The export routines of pyerrors are written such that as much information as possible is written automatically as described in the following example

    \n\n
    \n
    my_obs = pe.Obs([samples], ["test_ensemble"])\nmy_obs.tag = "My observable"\n\npe.input.json.dump_to_json(my_obs, "test_output_file", description="This file contains a test observable")\n# For a single observable one can equivalently use the class method dump\nmy_obs.dump("test_output_file", description="This file contains a test observable")\n\ncheck = pe.input.json.load_json("test_output_file")\n\nprint(my_obs == check)\n> True\n
    \n
    \n\n

    The format also allows to directly write out the content of Corr objects or lists and arrays of Obs objects by passing the desired data to pyerrors.input.json.dump_to_json.

    \n\n

    json.gz format specification

    \n\n

    The first entries of the file provide optional auxiliary information:

    \n\n
      \n
    • program is a string that indicates which program was used to write the file.
    • \n
    • version is a string that specifies the version of the format.
    • \n
    • who is a string that specifies the user name of the creator of the file.
    • \n
    • date is a string and contains the creation date of the file.
    • \n
    • host is a string and contains the hostname of the machine where the file has been written.
    • \n
    • description contains information on the content of the file. This field is not filled automatically in pyerrors. The user is advised to provide as detailed information as possible in this field. Examples are: Input files of measurements or simulations, LaTeX formulae or references to publications to specify how the observables have been computed, details on the analysis strategy, ... This field may be any valid JSON type. Strings, arrays or objects (equivalent to dicts in python) are well suited to provide information.
    • \n
    \n\n

    The only necessary entry of the file is the field\n-obsdata, an array that contains the actual data.

    \n\n

    Each entry of the array belongs to a single structure of observables. Currently, these structures can be either of Obs, list, numpy.ndarray, Corr. All Obs inside a structure (with dimension > 0) have to be defined on the same set of configurations. Different structures, that are represented by entries of the array obsdata, are treated independently. Each entry of the array obsdata has the following required entries:

    \n\n
      \n
    • type is a string that specifies the type of the structure. This allows to parse the content to the correct form after reading the file. It is always possible to interpret the content as list of Obs.
    • \n
    • value is an array that contains the mean values of the Obs inside the structure.\nThe following entries are optional:
    • \n
    • layout is a string that specifies the layout of multi-dimensional structures. Examples are \"2, 2\" for a 2x2 dimensional matrix or \"64, 4, 4\" for a Corr with $T=64$ and 4x4 matrices on each time slices. \"1\" denotes a single Obs. Multi-dimensional structures are stored in row-major format (see below).
    • \n
    • tag is any JSON type. It contains additional information concerning the structure. The tag of an Obs in pyerrors is written here.
    • \n
    • reweighted is a Bool that may be used to specify, whether the Obs in the structure have been reweighted.
    • \n
    • data is an array that contains the data from MC chains. We will define it below.
    • \n
    • cdata is an array that contains the data from external quantities with an error (Covobs in pyerrors). We will define it below.
    • \n
    \n\n

    The array data contains the data from MC chains. Each entry of the array corresponds to one ensemble and contains:

    \n\n
      \n
    • id, a string that contains the name of the ensemble
    • \n
    • replica, an array that contains an entry per replica of the ensemble.
    • \n
    \n\n

    Each entry of replica contains\nname, a string that contains the name of the replica\ndeltas, an array that contains the actual data.

    \n\n

    Each entry in deltas corresponds to one configuration of the replica and has $1+N$ many entries. The first entry is an integer that specifies the configuration number that, together with ensemble and replica name, may be used to uniquely identify the configuration on which the data has been obtained. The following N entries specify the deltas, i.e., the deviation of the observable from the mean value on this configuration, of each Obs inside the structure. Multi-dimensional structures are stored in a row-major format. For primary observables, such as correlation functions, $value + delta_i$ matches the primary data obtained on the configuration.

    \n\n

    The array cdata contains information about the contribution of auxiliary observables, represented by Covobs in pyerrors, to the total error of the observables. Each entry of the array belongs to one auxiliary covariance matrix and contains:

    \n\n
      \n
    • id, a string that identifies the covariance matrix
    • \n
    • layout, a string that defines the dimensions of the $M\\times M$ covariance matrix (has to be \"M, M\" or \"1\").
    • \n
    • cov, an array that contains the $M\\times M$ many entries of the covariance matrix, stored in row-major format.
    • \n
    • grad, an array that contains N entries, one for each Obs inside the structure. Each entry itself is an array, that contains the M gradients of the Nth observable with respect to the quantity that corresponds to the Mth diagonal entry of the covariance matrix.
    • \n
    \n\n

    A JSON schema that may be used to verify the correctness of a file with respect to the format definition is stored in ./examples/json_schema.json. The schema is a self-descriptive format definition and contains an exemplary file.

    \n\n

    Julia I/O routines for the json.gz format, compatible with ADerrors.jl, can be found here.

    \n"}, "pyerrors.correlators": {"fullname": "pyerrors.correlators", "modulename": "pyerrors.correlators", "kind": "module", "doc": "

    \n"}, "pyerrors.correlators.Corr": {"fullname": "pyerrors.correlators.Corr", "modulename": "pyerrors.correlators", "qualname": "Corr", "kind": "class", "doc": "

    The class for a correlator (time dependent sequence of pe.Obs).

    \n\n

    Everything, this class does, can be achieved using lists or arrays of Obs.\nBut it is simply more convenient to have a dedicated object for correlators.\nOne often wants to add or multiply correlators of the same length at every timeslice and it is inconvenient\nto iterate over all timeslices for every operation. This is especially true, when dealing with matrices.

    \n\n

    The correlator can have two types of content: An Obs at every timeslice OR a GEVP\nmatrix at every timeslice. Other dependency (eg. spatial) are not supported.

    \n"}, "pyerrors.correlators.Corr.__init__": {"fullname": "pyerrors.correlators.Corr.__init__", "modulename": "pyerrors.correlators", "qualname": "Corr.__init__", "kind": "function", "doc": "

    Initialize a Corr object.

    \n\n
    Parameters
    \n\n
      \n
    • data_input (list or array):\nlist of Obs or list of arrays of Obs or array of Corrs
    • \n
    • padding (list, optional):\nList with two entries where the first labels the padding\nat the front of the correlator and the second the padding\nat the back.
    • \n
    • prange (list, optional):\nList containing the first and last timeslice of the plateau\nregion indentified for this correlator.
    • \n
    \n", "signature": "(data_input, padding=[0, 0], prange=None)"}, "pyerrors.correlators.Corr.gamma_method": {"fullname": "pyerrors.correlators.Corr.gamma_method", "modulename": "pyerrors.correlators", "qualname": "Corr.gamma_method", "kind": "function", "doc": "

    Apply the gamma method to the content of the Corr.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.gm": {"fullname": "pyerrors.correlators.Corr.gm", "modulename": "pyerrors.correlators", "qualname": "Corr.gm", "kind": "function", "doc": "

    Apply the gamma method to the content of the Corr.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.projected": {"fullname": "pyerrors.correlators.Corr.projected", "modulename": "pyerrors.correlators", "qualname": "Corr.projected", "kind": "function", "doc": "

    We need to project the Correlator with a Vector to get a single value at each timeslice.

    \n\n

    The method can use one or two vectors.\nIf two are specified it returns v1@G@v2 (the order might be very important.)\nBy default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to

    \n", "signature": "(self, vector_l=None, vector_r=None, normalize=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.item": {"fullname": "pyerrors.correlators.Corr.item", "modulename": "pyerrors.correlators", "qualname": "Corr.item", "kind": "function", "doc": "

    Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice.

    \n\n
    Parameters
    \n\n
      \n
    • i (int):\nFirst index to be picked.
    • \n
    • j (int):\nSecond index to be picked.
    • \n
    \n", "signature": "(self, i, j):", "funcdef": "def"}, "pyerrors.correlators.Corr.plottable": {"fullname": "pyerrors.correlators.Corr.plottable", "modulename": "pyerrors.correlators", "qualname": "Corr.plottable", "kind": "function", "doc": "

    Outputs the correlator in a plotable format.

    \n\n

    Outputs three lists containing the timeslice index, the value on each\ntimeslice and the error on each timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.symmetric": {"fullname": "pyerrors.correlators.Corr.symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.symmetric", "kind": "function", "doc": "

    Symmetrize the correlator around x0=0.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.anti_symmetric": {"fullname": "pyerrors.correlators.Corr.anti_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.anti_symmetric", "kind": "function", "doc": "

    Anti-symmetrize the correlator around x0=0.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.is_matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.is_matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.is_matrix_symmetric", "kind": "function", "doc": "

    Checks whether a correlator matrices is symmetric on every timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.matrix_symmetric", "kind": "function", "doc": "

    Symmetrizes the correlator matrices on every timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.GEVP": {"fullname": "pyerrors.correlators.Corr.GEVP", "modulename": "pyerrors.correlators", "qualname": "Corr.GEVP", "kind": "function", "doc": "

    Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors.

    \n\n

    The eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the\nlargest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing

    \n\n
    \n
    C.GEVP(t0=2)[0]  # Ground state vector(s)\nC.GEVP(t0=2)[:3]  # Vectors for the lowest three states\n
    \n
    \n\n
    Parameters
    \n\n
      \n
    • t0 (int):\nThe time t0 for the right hand side of the GEVP according to $G(t)v_i=\\lambda_i G(t_0)v_i$
    • \n
    • ts (int):\nfixed time $G(t_s)v_i=\\lambda_i G(t_0)v_i$ if sort=None.\nIf sort=\"Eigenvector\" it gives a reference point for the sorting method.
    • \n
    • sort (string):\nIf this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned.\n
        \n
      • \"Eigenvalue\": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice.
      • \n
      • \"Eigenvector\": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state.\nThe reference state is identified by its eigenvalue at $t=t_s$.
      • \n
    • \n
    \n\n
    Other Parameters
    \n\n
      \n
    • state (int):\nReturns only the vector(s) for a specified state. The lowest state is zero.
    • \n
    \n", "signature": "(self, t0, ts=None, sort='Eigenvalue', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.Eigenvalue": {"fullname": "pyerrors.correlators.Corr.Eigenvalue", "modulename": "pyerrors.correlators", "qualname": "Corr.Eigenvalue", "kind": "function", "doc": "

    Determines the eigenvalue of the GEVP by solving and projecting the correlator

    \n\n
    Parameters
    \n\n
      \n
    • state (int):\nThe state one is interested in ordered by energy. The lowest state is zero.
    • \n
    • All other parameters are identical to the ones of Corr.GEVP.
    • \n
    \n", "signature": "(self, t0, ts=None, state=0, sort='Eigenvalue'):", "funcdef": "def"}, "pyerrors.correlators.Corr.Hankel": {"fullname": "pyerrors.correlators.Corr.Hankel", "modulename": "pyerrors.correlators", "qualname": "Corr.Hankel", "kind": "function", "doc": "

    Constructs an NxN Hankel matrix

    \n\n

    C(t) c(t+1) ... c(t+n-1)\nC(t+1) c(t+2) ... c(t+n)\n.................\nC(t+(n-1)) c(t+n) ... c(t+2(n-1))

    \n\n
    Parameters
    \n\n
      \n
    • N (int):\nDimension of the Hankel matrix
    • \n
    • periodic (bool, optional):\ndetermines whether the matrix is extended periodically
    • \n
    \n", "signature": "(self, N, periodic=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.roll": {"fullname": "pyerrors.correlators.Corr.roll", "modulename": "pyerrors.correlators", "qualname": "Corr.roll", "kind": "function", "doc": "

    Periodically shift the correlator by dt timeslices

    \n\n
    Parameters
    \n\n
      \n
    • dt (int):\nnumber of timeslices
    • \n
    \n", "signature": "(self, dt):", "funcdef": "def"}, "pyerrors.correlators.Corr.reverse": {"fullname": "pyerrors.correlators.Corr.reverse", "modulename": "pyerrors.correlators", "qualname": "Corr.reverse", "kind": "function", "doc": "

    Reverse the time ordering of the Corr

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.thin": {"fullname": "pyerrors.correlators.Corr.thin", "modulename": "pyerrors.correlators", "qualname": "Corr.thin", "kind": "function", "doc": "

    Thin out a correlator to suppress correlations

    \n\n
    Parameters
    \n\n
      \n
    • spacing (int):\nKeep only every 'spacing'th entry of the correlator
    • \n
    • offset (int):\nOffset the equal spacing
    • \n
    \n", "signature": "(self, spacing=2, offset=0):", "funcdef": "def"}, "pyerrors.correlators.Corr.correlate": {"fullname": "pyerrors.correlators.Corr.correlate", "modulename": "pyerrors.correlators", "qualname": "Corr.correlate", "kind": "function", "doc": "

    Correlate the correlator with another correlator or Obs

    \n\n
    Parameters
    \n\n
      \n
    • partner (Obs or Corr):\npartner to correlate the correlator with.\nCan either be an Obs which is correlated with all entries of the\ncorrelator or a Corr of same length.
    • \n
    \n", "signature": "(self, partner):", "funcdef": "def"}, "pyerrors.correlators.Corr.reweight": {"fullname": "pyerrors.correlators.Corr.reweight", "modulename": "pyerrors.correlators", "qualname": "Corr.reweight", "kind": "function", "doc": "

    Reweight the correlator.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl.
    • \n
    \n", "signature": "(self, weight, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.T_symmetry": {"fullname": "pyerrors.correlators.Corr.T_symmetry", "modulename": "pyerrors.correlators", "qualname": "Corr.T_symmetry", "kind": "function", "doc": "

    Return the time symmetry average of the correlator and its partner

    \n\n
    Parameters
    \n\n
      \n
    • partner (Corr):\nTime symmetry partner of the Corr
    • \n
    • partity (int):\nParity quantum number of the correlator, can be +1 or -1
    • \n
    \n", "signature": "(self, partner, parity=1):", "funcdef": "def"}, "pyerrors.correlators.Corr.deriv": {"fullname": "pyerrors.correlators.Corr.deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.deriv", "kind": "function", "doc": "

    Return the first derivative of the correlator with respect to x0.

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, forward, backward, improved, log, default: symmetric
    • \n
    \n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.second_deriv": {"fullname": "pyerrors.correlators.Corr.second_deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.second_deriv", "kind": "function", "doc": "

    Return the second derivative of the correlator with respect to x0.

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, improved, log, default: symmetric
    • \n
    \n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.m_eff": {"fullname": "pyerrors.correlators.Corr.m_eff", "modulename": "pyerrors.correlators", "qualname": "Corr.m_eff", "kind": "function", "doc": "

    Returns the effective mass of the correlator as correlator object

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\nlog : uses the standard effective mass log(C(t) / C(t+1))\ncosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m.\nsinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m.\nSee, e.g., arXiv:1205.5380\narccosh : Uses the explicit form of the symmetrized correlator (not recommended)\nlogsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2
    • \n
    • guess (float):\nguess for the root finder, only relevant for the root variant
    • \n
    \n", "signature": "(self, variant='log', guess=1.0):", "funcdef": "def"}, "pyerrors.correlators.Corr.fit": {"fullname": "pyerrors.correlators.Corr.fit", "modulename": "pyerrors.correlators", "qualname": "Corr.fit", "kind": "function", "doc": "

    Fits function to the data

    \n\n
    Parameters
    \n\n
      \n
    • function (obj):\nfunction to fit to the data. See fits.least_squares for details.
    • \n
    • fitrange (list):\nTwo element list containing the timeslices on which the fit is supposed to start and stop.\nCaution: This range is inclusive as opposed to standard python indexing.\nfitrange=[4, 6] corresponds to the three entries 4, 5 and 6.\nIf not specified, self.prange or all timeslices are used.
    • \n
    • silent (bool):\nDecides whether output is printed to the standard output.
    • \n
    \n", "signature": "(self, function, fitrange=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.plateau": {"fullname": "pyerrors.correlators.Corr.plateau", "modulename": "pyerrors.correlators", "qualname": "Corr.plateau", "kind": "function", "doc": "

    Extract a plateau value from a Corr object

    \n\n
    Parameters
    \n\n
      \n
    • plateau_range (list):\nlist with two entries, indicating the first and the last timeslice\nof the plateau region.
    • \n
    • method (str):\nmethod to extract the plateau.\n 'fit' fits a constant to the plateau region\n 'avg', 'average' or 'mean' just average over the given timeslices.
    • \n
    • auto_gamma (bool):\napply gamma_method with default parameters to the Corr. Defaults to None
    • \n
    \n", "signature": "(self, plateau_range=None, method='fit', auto_gamma=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.set_prange": {"fullname": "pyerrors.correlators.Corr.set_prange", "modulename": "pyerrors.correlators", "qualname": "Corr.set_prange", "kind": "function", "doc": "

    Sets the attribute prange of the Corr object.

    \n", "signature": "(self, prange):", "funcdef": "def"}, "pyerrors.correlators.Corr.show": {"fullname": "pyerrors.correlators.Corr.show", "modulename": "pyerrors.correlators", "qualname": "Corr.show", "kind": "function", "doc": "

    Plots the correlator using the tag of the correlator as label if available.

    \n\n
    Parameters
    \n\n
      \n
    • x_range (list):\nlist of two values, determining the range of the x-axis e.g. [4, 8].
    • \n
    • comp (Corr or list of Corr):\nCorrelator or list of correlators which are plotted for comparison.\nThe tags of these correlators are used as labels if available.
    • \n
    • logscale (bool):\nSets y-axis to logscale.
    • \n
    • plateau (Obs):\nPlateau value to be visualized in the figure.
    • \n
    • fit_res (Fit_result):\nFit_result object to be visualized.
    • \n
    • fit_key (str):\nKey for the fit function in Fit_result.fit_function (for combined fits).
    • \n
    • ylabel (str):\nLabel for the y-axis.
    • \n
    • save (str):\npath to file in which the figure should be saved.
    • \n
    • auto_gamma (bool):\nApply the gamma method with standard parameters to all correlators and plateau values before plotting.
    • \n
    • hide_sigma (float):\nHides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors.
    • \n
    • references (list):\nList of floating point values that are displayed as horizontal lines for reference.
    • \n
    • title (string):\nOptional title of the figure.
    • \n
    \n", "signature": "(\tself,\tx_range=None,\tcomp=None,\ty_range=None,\tlogscale=False,\tplateau=None,\tfit_res=None,\tfit_key=None,\tylabel=None,\tsave=None,\tauto_gamma=False,\thide_sigma=None,\treferences=None,\ttitle=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.spaghetti_plot": {"fullname": "pyerrors.correlators.Corr.spaghetti_plot", "modulename": "pyerrors.correlators", "qualname": "Corr.spaghetti_plot", "kind": "function", "doc": "

    Produces a spaghetti plot of the correlator suited to monitor exceptional configurations.

    \n\n
    Parameters
    \n\n
      \n
    • logscale (bool):\nDetermines whether the scale of the y-axis is logarithmic or standard.
    • \n
    \n", "signature": "(self, logscale=True):", "funcdef": "def"}, "pyerrors.correlators.Corr.dump": {"fullname": "pyerrors.correlators.Corr.dump", "modulename": "pyerrors.correlators", "qualname": "Corr.dump", "kind": "function", "doc": "

    Dumps the Corr into a file of chosen type

    \n\n
    Parameters
    \n\n
      \n
    • filename (str):\nName of the file to be saved.
    • \n
    • datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n", "signature": "(self, filename, datatype='json.gz', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.print": {"fullname": "pyerrors.correlators.Corr.print", "modulename": "pyerrors.correlators", "qualname": "Corr.print", "kind": "function", "doc": "

    \n", "signature": "(self, print_range=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.sqrt": {"fullname": "pyerrors.correlators.Corr.sqrt", "modulename": "pyerrors.correlators", "qualname": "Corr.sqrt", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.log": {"fullname": "pyerrors.correlators.Corr.log", "modulename": "pyerrors.correlators", "qualname": "Corr.log", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.exp": {"fullname": "pyerrors.correlators.Corr.exp", "modulename": "pyerrors.correlators", "qualname": "Corr.exp", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sin": {"fullname": "pyerrors.correlators.Corr.sin", "modulename": "pyerrors.correlators", "qualname": "Corr.sin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cos": {"fullname": "pyerrors.correlators.Corr.cos", "modulename": "pyerrors.correlators", "qualname": "Corr.cos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tan": {"fullname": "pyerrors.correlators.Corr.tan", "modulename": "pyerrors.correlators", "qualname": "Corr.tan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sinh": {"fullname": "pyerrors.correlators.Corr.sinh", "modulename": "pyerrors.correlators", "qualname": "Corr.sinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cosh": {"fullname": "pyerrors.correlators.Corr.cosh", "modulename": "pyerrors.correlators", "qualname": "Corr.cosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tanh": {"fullname": "pyerrors.correlators.Corr.tanh", "modulename": "pyerrors.correlators", "qualname": "Corr.tanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsin": {"fullname": "pyerrors.correlators.Corr.arcsin", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccos": {"fullname": "pyerrors.correlators.Corr.arccos", "modulename": "pyerrors.correlators", "qualname": "Corr.arccos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctan": {"fullname": "pyerrors.correlators.Corr.arctan", "modulename": "pyerrors.correlators", "qualname": "Corr.arctan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsinh": {"fullname": "pyerrors.correlators.Corr.arcsinh", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccosh": {"fullname": "pyerrors.correlators.Corr.arccosh", "modulename": "pyerrors.correlators", "qualname": "Corr.arccosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctanh": {"fullname": "pyerrors.correlators.Corr.arctanh", "modulename": "pyerrors.correlators", "qualname": "Corr.arctanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.prune": {"fullname": "pyerrors.correlators.Corr.prune", "modulename": "pyerrors.correlators", "qualname": "Corr.prune", "kind": "function", "doc": "

    Project large correlation matrix to lowest states

    \n\n

    This method can be used to reduce the size of an (N x N) correlation matrix\nto (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise\nis still small.

    \n\n
    Parameters
    \n\n
      \n
    • Ntrunc (int):\nRank of the target matrix.
    • \n
    • tproj (int):\nTime where the eigenvectors are evaluated, corresponds to ts in the GEVP method.\nThe default value is 3.
    • \n
    • t0proj (int):\nTime where the correlation matrix is inverted. Choosing t0proj=1 is strongly\ndiscouraged for O(a) improved theories, since the correctness of the procedure\ncannot be granted in this case. The default value is 2.
    • \n
    • basematrix (Corr):\nCorrelation matrix that is used to determine the eigenvectors of the\nlowest states based on a GEVP. basematrix is taken to be the Corr itself if\nis is not specified.
    • \n
    \n\n
    Notes
    \n\n

    We have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving\nthe GEVP $$C(t) v_n(t, t_0) = \\lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \\equiv t_\\mathrm{proj}$\nand $t_0 \\equiv t_{0, \\mathrm{proj}}$. The target matrix is projected onto the subspace of the\nresulting eigenvectors $v_n, n=1,\\dots,N_\\mathrm{trunc}$ via\n$$G^\\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large\ncorrelation matrix and to remove some noise that is added by irrelevant operators.\nThis may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated\nbound $t_0 \\leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$.

    \n", "signature": "(self, Ntrunc, tproj=3, t0proj=2, basematrix=None):", "funcdef": "def"}, "pyerrors.covobs": {"fullname": "pyerrors.covobs", "modulename": "pyerrors.covobs", "kind": "module", "doc": "

    \n"}, "pyerrors.covobs.Covobs": {"fullname": "pyerrors.covobs.Covobs", "modulename": "pyerrors.covobs", "qualname": "Covobs", "kind": "class", "doc": "

    \n"}, "pyerrors.covobs.Covobs.__init__": {"fullname": "pyerrors.covobs.Covobs.__init__", "modulename": "pyerrors.covobs", "qualname": "Covobs.__init__", "kind": "function", "doc": "

    Initialize Covobs object.

    \n\n
    Parameters
    \n\n
      \n
    • mean (float):\nMean value of the new Obs
    • \n
    • cov (list or array):\n2d Covariance matrix or 1d diagonal entries
    • \n
    • name (str):\nidentifier for the covariance matrix
    • \n
    • pos (int):\nPosition of the variance belonging to mean in cov.\nIs taken to be 1 if cov is 0-dimensional
    • \n
    • grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
    • \n
    \n", "signature": "(mean, cov, name, pos=None, grad=None)"}, "pyerrors.covobs.Covobs.errsq": {"fullname": "pyerrors.covobs.Covobs.errsq", "modulename": "pyerrors.covobs", "qualname": "Covobs.errsq", "kind": "function", "doc": "

    Return the variance (= square of the error) of the Covobs

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.dirac": {"fullname": "pyerrors.dirac", "modulename": "pyerrors.dirac", "kind": "module", "doc": "

    \n"}, "pyerrors.dirac.epsilon_tensor": {"fullname": "pyerrors.dirac.epsilon_tensor", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor", "kind": "function", "doc": "

    Rank-3 epsilon tensor

    \n\n

    Based on https://codegolf.stackexchange.com/a/160375

    \n\n
    Returns
    \n\n
      \n
    • elem (int):\nElement (i,j,k) of the epsilon tensor of rank 3
    • \n
    \n", "signature": "(i, j, k):", "funcdef": "def"}, "pyerrors.dirac.epsilon_tensor_rank4": {"fullname": "pyerrors.dirac.epsilon_tensor_rank4", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor_rank4", "kind": "function", "doc": "

    Rank-4 epsilon tensor

    \n\n

    Extension of https://codegolf.stackexchange.com/a/160375

    \n\n
    Returns
    \n\n
      \n
    • elem (int):\nElement (i,j,k,o) of the epsilon tensor of rank 4
    • \n
    \n", "signature": "(i, j, k, o):", "funcdef": "def"}, "pyerrors.dirac.Grid_gamma": {"fullname": "pyerrors.dirac.Grid_gamma", "modulename": "pyerrors.dirac", "qualname": "Grid_gamma", "kind": "function", "doc": "

    Returns gamma matrix in Grid labeling.

    \n", "signature": "(gamma_tag):", "funcdef": "def"}, "pyerrors.fits": {"fullname": "pyerrors.fits", "modulename": "pyerrors.fits", "kind": "module", "doc": "

    \n"}, "pyerrors.fits.Fit_result": {"fullname": "pyerrors.fits.Fit_result", "modulename": "pyerrors.fits", "qualname": "Fit_result", "kind": "class", "doc": "

    Represents fit results.

    \n\n
    Attributes
    \n\n
      \n
    • fit_parameters (list):\nresults for the individual fit parameters,\nalso accessible via indices.
    • \n
    • chisquare_by_dof (float):\nreduced chisquare.
    • \n
    • p_value (float):\np-value of the fit
    • \n
    • t2_p_value (float):\nHotelling t-squared p-value for correlated fits.
    • \n
    \n", "bases": "collections.abc.Sequence"}, "pyerrors.fits.Fit_result.gamma_method": {"fullname": "pyerrors.fits.Fit_result.gamma_method", "modulename": "pyerrors.fits", "qualname": "Fit_result.gamma_method", "kind": "function", "doc": "

    Apply the gamma method to all fit parameters

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.Fit_result.gm": {"fullname": "pyerrors.fits.Fit_result.gm", "modulename": "pyerrors.fits", "qualname": "Fit_result.gm", "kind": "function", "doc": "

    Apply the gamma method to all fit parameters

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.least_squares": {"fullname": "pyerrors.fits.least_squares", "modulename": "pyerrors.fits", "qualname": "least_squares", "kind": "function", "doc": "

    Performs a non-linear fit to y = func(x).\n ```

    \n\n
    Parameters
    \n\n
      \n
    • For an uncombined fit:
    • \n
    • x (list):\nlist of floats.
    • \n
    • y (list):\nlist of Obs.
    • \n
    • func (object):\nfit function, has to be of the form

      \n\n
      \n
      import autograd.numpy as anp\n\ndef func(a, x):\n   return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
      \n
      \n\n

      For multiple x values func can be of the form

      \n\n
      \n
      def func(a, x):\n   (x1, x2) = x\n   return a[0] * x1 ** 2 + a[1] * x2\n
      \n
      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • OR For a combined fit:
    • \n
    • x (dict):\ndict of lists.
    • \n
    • y (dict):\ndict of lists of Obs.
    • \n
    • funcs (dict):\ndict of objects\nfit functions have to be of the form (here a[0] is the common fit parameter)\n```python\nimport autograd.numpy as anp\nfuncs = {\"a\": func_a,\n \"b\": func_b}

      \n\n

      def func_a(a, x):\n return a[1] * anp.exp(-a[0] * x)

      \n\n

      def func_b(a, x):\n return a[2] * anp.exp(-a[0] * x)

      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • priors (dict or list, optional):\npriors can either be a dictionary with integer keys and the corresponding priors as values or\na list with an entry for every parameter in the fit. The entries can either be\nObs (e.g. results from a previous fit) or strings containing a value and an error formatted like\n0.548(23), 500(40) or 0.5(0.4)
    • \n
    • silent (bool, optional):\nIf true all output to the console is omitted (default False).
    • \n
    • initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for\nnon-linear fits with many parameters. In case of correlated fits the guess is used to perform\nan uncorrelated fit which then serves as guess for the correlated fit.
    • \n
    • method (str, optional):\ncan be used to choose an alternative method for the minimization of chisquare.\nThe possible methods are the ones which can be used for scipy.optimize.minimize and\nmigrad of iminuit. If no method is specified, Levenberg-Marquard is used.\nReliable alternatives are migrad, Powell and Nelder-Mead.
    • \n
    • tol (float, optional):\ncan be used (only for combined fits and methods other than Levenberg-Marquard) to set the tolerance for convergence\nto a different value to either speed up convergence at the cost of a larger error on the fitted parameters (and possibly\ninvalid estimates for parameter uncertainties) or smaller values to get more accurate parameter values\nThe stopping criterion depends on the method, e.g. migrad: edm_max = 0.002 * tol * errordef (EDM criterion: edm < edm_max)
    • \n
    • correlated_fit (bool):\nIf True, use the full inverse covariance matrix in the definition of the chisquare cost function.\nFor details about how the covariance matrix is estimated see pyerrors.obs.covariance.\nIn practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix).\nThis procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning).
    • \n
    • expected_chisquare (bool):\nIf True estimates the expected chisquare which is\ncorrected by effects caused by correlated input data (default False).
    • \n
    • resplot (bool):\nIf True, a plot which displays fit, data and residuals is generated (default False).
    • \n
    • qqplot (bool):\nIf True, a quantile-quantile plot of the fit result is generated (default False).
    • \n
    • num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • output (Fit_result):\nParameters and information on the fitted result.
    • \n
    \n", "signature": "(x, y, func, priors=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.total_least_squares": {"fullname": "pyerrors.fits.total_least_squares", "modulename": "pyerrors.fits", "qualname": "total_least_squares", "kind": "function", "doc": "

    Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters.

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nlist of Obs, or a tuple of lists of Obs
    • \n
    • y (list):\nlist of Obs. The dvalues of the Obs are used as x- and yerror for the fit.
    • \n
    • func (object):\nfunc has to be of the form

      \n\n
      \n
      import autograd.numpy as anp\n\ndef func(a, x):\n   return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
      \n
      \n\n

      For multiple x values func can be of the form

      \n\n
      \n
      def func(a, x):\n   (x1, x2) = x\n   return a[0] * x1 ** 2 + a[1] * x2\n
      \n
      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • silent (bool, optional):\nIf true all output to the console is omitted (default False).
    • \n
    • initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for non-linear\nfits with many parameters.
    • \n
    • expected_chisquare (bool):\nIf true prints the expected chisquare which is\ncorrected by effects caused by correlated input data.\nThis can take a while as the full correlation matrix\nhas to be calculated (default False).
    • \n
    • num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
    • \n
    \n\n
    Notes
    \n\n

    Based on the orthogonal distance regression module of scipy.

    \n\n
    Returns
    \n\n
      \n
    • output (Fit_result):\nParameters and information on the fitted result.
    • \n
    \n", "signature": "(x, y, func, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.fit_lin": {"fullname": "pyerrors.fits.fit_lin", "modulename": "pyerrors.fits", "qualname": "fit_lin", "kind": "function", "doc": "

    Performs a linear fit to y = n + m * x and returns two Obs n, m.

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nCan either be a list of floats in which case no xerror is assumed, or\na list of Obs, where the dvalues of the Obs are used as xerror for the fit.
    • \n
    • y (list):\nList of Obs, the dvalues of the Obs are used as yerror for the fit.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • fit_parameters (list[Obs]):\nLIist of fitted observables.
    • \n
    \n", "signature": "(x, y, **kwargs):", "funcdef": "def"}, "pyerrors.fits.qqplot": {"fullname": "pyerrors.fits.qqplot", "modulename": "pyerrors.fits", "qualname": "qqplot", "kind": "function", "doc": "

    Generates a quantile-quantile plot of the fit result which can be used to\n check if the residuals of the fit are gaussian distributed.

    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(x, o_y, func, p, title=''):", "funcdef": "def"}, "pyerrors.fits.residual_plot": {"fullname": "pyerrors.fits.residual_plot", "modulename": "pyerrors.fits", "qualname": "residual_plot", "kind": "function", "doc": "

    Generates a plot which compares the fit to the data and displays the corresponding residuals

    \n\n

    For uncorrelated data the residuals are expected to be distributed ~N(0,1).

    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(x, y, func, fit_res, title=''):", "funcdef": "def"}, "pyerrors.fits.error_band": {"fullname": "pyerrors.fits.error_band", "modulename": "pyerrors.fits", "qualname": "error_band", "kind": "function", "doc": "

    Calculate the error band for an array of sample values x, for given fit function func with optimized parameters beta.

    \n\n
    Returns
    \n\n
      \n
    • err (np.array(Obs)):\nError band for an array of sample values x
    • \n
    \n", "signature": "(x, func, beta):", "funcdef": "def"}, "pyerrors.fits.ks_test": {"fullname": "pyerrors.fits.ks_test", "modulename": "pyerrors.fits", "qualname": "ks_test", "kind": "function", "doc": "

    Performs a Kolmogorov\u2013Smirnov test for the p-values of all fit object.

    \n\n
    Parameters
    \n\n
      \n
    • objects (list):\nList of fit results to include in the analysis (optional).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(objects=None):", "funcdef": "def"}, "pyerrors.input": {"fullname": "pyerrors.input", "modulename": "pyerrors.input", "kind": "module", "doc": "

    pyerrors includes an input submodule in which input routines and parsers for the output of various numerical programs are contained.

    \n\n

    Jackknife samples

    \n\n

    For comparison with other analysis workflows pyerrors can also generate jackknife samples from an Obs object or import jackknife samples into an Obs object.\nSee pyerrors.obs.Obs.export_jackknife and pyerrors.obs.import_jackknife for details.

    \n"}, "pyerrors.input.bdio": {"fullname": "pyerrors.input.bdio", "modulename": "pyerrors.input.bdio", "kind": "module", "doc": "

    \n"}, "pyerrors.input.bdio.read_ADerrors": {"fullname": "pyerrors.input.bdio.read_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "read_ADerrors", "kind": "function", "doc": "

    Extract generic MCMC data from a bdio file

    \n\n

    read_ADerrors requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path -- path to the bdio file
    • \n
    • bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (List[Obs]):\nExtracted data
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.write_ADerrors": {"fullname": "pyerrors.input.bdio.write_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "write_ADerrors", "kind": "function", "doc": "

    Write Obs to a bdio file according to ADerrors conventions

    \n\n

    read_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path -- path to the bdio file
    • \n
    • bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • success (int):\nreturns 0 is successful
    • \n
    \n", "signature": "(obs_list, file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_mesons": {"fullname": "pyerrors.input.bdio.read_mesons", "modulename": "pyerrors.input.bdio", "qualname": "read_mesons", "kind": "function", "doc": "

    Extract mesons data from a bdio file and return it as a dictionary

    \n\n

    The dictionary can be accessed with a tuple consisting of (type, source_position, kappa1, kappa2)

    \n\n

    read_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path (str):\npath to the bdio file
    • \n
    • bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    • start (int):\nThe first configuration to be read (default 1)
    • \n
    • stop (int):\nThe last configuration to be read (default None)
    • \n
    • step (int):\nFixed step size between two measurements (default 1)
    • \n
    • alternative_ensemble_name (str):\nManually overwrite ensemble name
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (dict):\nExtracted meson data
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_dSdm": {"fullname": "pyerrors.input.bdio.read_dSdm", "modulename": "pyerrors.input.bdio", "qualname": "read_dSdm", "kind": "function", "doc": "

    Extract dSdm data from a bdio file and return it as a dictionary

    \n\n

    The dictionary can be accessed with a tuple consisting of (type, kappa)

    \n\n

    read_dSdm requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path (str):\npath to the bdio file
    • \n
    • bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    • start (int):\nThe first configuration to be read (default 1)
    • \n
    • stop (int):\nThe last configuration to be read (default None)
    • \n
    • step (int):\nFixed step size between two measurements (default 1)
    • \n
    • alternative_ensemble_name (str):\nManually overwrite ensemble name
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.dobs": {"fullname": "pyerrors.input.dobs", "modulename": "pyerrors.input.dobs", "kind": "module", "doc": "

    \n"}, "pyerrors.input.dobs.create_pobs_string": {"fullname": "pyerrors.input.dobs.create_pobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_pobs_string", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to an xml string\naccording to the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • xml_str (str):\nXML formatted string of the input data
    • \n
    \n", "signature": "(obsl, name, spec='', origin='', symbol=[], enstag=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_pobs": {"fullname": "pyerrors.input.dobs.write_pobs", "modulename": "pyerrors.input.dobs", "qualname": "write_pobs", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
    • \n
    • gz (bool):\nIf True, the output is a gzipped xml. If False, the output is an xml file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(\tobsl,\tfname,\tname,\tspec='',\torigin='',\tsymbol=[],\tenstag=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_pobs": {"fullname": "pyerrors.input.dobs.read_pobs", "modulename": "pyerrors.input.dobs", "qualname": "read_pobs", "kind": "function", "doc": "

    Import a list of Obs from an xml.gz file in the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • separatior_insertion (str or int):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nNone (default): Replica names remain unchanged.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(fname, full_output=False, gz=True, separator_insertion=None):", "funcdef": "def"}, "pyerrors.input.dobs.import_dobs_string": {"fullname": "pyerrors.input.dobs.import_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "import_dobs_string", "kind": "function", "doc": "

    Import a list of Obs from a string in the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • content (str):\nXML string containing the data
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(content, full_output=False, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_dobs": {"fullname": "pyerrors.input.dobs.read_dobs", "modulename": "pyerrors.input.dobs", "qualname": "read_dobs", "kind": "function", "doc": "

    Import a list of Obs from an xml.gz file in the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes XML file.
    • \n
    • separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(fname, full_output=False, gz=True, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.create_dobs_string": {"fullname": "pyerrors.input.dobs.create_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_dobs_string", "kind": "function", "doc": "

    Generate the string for the export of a list of Obs or structures containing Obs\nto a .xml.gz file according to the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically. The separator |is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • who (str):\nProvide the name of the person that exports the data.
    • \n
    • enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • xml_str (str):\nXML string generated from the data
    • \n
    \n", "signature": "(\tobsl,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_dobs": {"fullname": "pyerrors.input.dobs.write_dobs", "modulename": "pyerrors.input.dobs", "qualname": "write_dobs", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • who (str):\nProvide the name of the person that exports the data.
    • \n
    • enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
    • \n
    • gz (bool):\nIf True, the output is a gzipped XML. If False, the output is a XML file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(\tobsl,\tfname,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.hadrons": {"fullname": "pyerrors.input.hadrons", "modulename": "pyerrors.input.hadrons", "kind": "module", "doc": "

    \n"}, "pyerrors.input.hadrons.read_meson_hd5": {"fullname": "pyerrors.input.hadrons.read_meson_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_meson_hd5", "kind": "function", "doc": "

    Read hadrons meson hdf5 file and extract the meson labeled 'meson'

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • meson (str):\nlabel of the meson to be extracted, standard value meson_0 which\ncorresponds to the pseudoscalar pseudoscalar two-point function.
    • \n
    • gammas (tuple of strings):\nInstrad of a meson label one can also provide a tuple of two strings\nindicating the gamma matrices at source and sink.\n(\"Gamma5\", \"Gamma5\") corresponds to the pseudoscalar pseudoscalar\ntwo-point function. The gammas argument dominateds over meson.
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • corr (Corr):\nCorrelator of the source sink combination in question.
    • \n
    \n", "signature": "(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_DistillationContraction_hd5": {"fullname": "pyerrors.input.hadrons.read_DistillationContraction_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_DistillationContraction_hd5", "kind": "function", "doc": "

    Read hadrons DistillationContraction hdf5 files in given directory structure

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the directories to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • diagrams (list):\nList of strings of the diagrams to extract, e.g. [\"direct\", \"box\", \"cross\"].
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (dict):\nextracted DistillationContration data
    • \n
    \n", "signature": "(path, ens_id, diagrams=['direct'], idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.Npr_matrix": {"fullname": "pyerrors.input.hadrons.Npr_matrix", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix", "kind": "class", "doc": "

    ndarray(shape, dtype=float, buffer=None, offset=0,\n strides=None, order=None)

    \n\n

    An array object represents a multidimensional, homogeneous array\nof fixed-size items. An associated data-type object describes the\nformat of each element in the array (its byte-order, how many bytes it\noccupies in memory, whether it is an integer, a floating point number,\nor something else, etc.)

    \n\n

    Arrays should be constructed using array, zeros or empty (refer\nto the See Also section below). The parameters given here refer to\na low-level method (ndarray(...)) for instantiating an array.

    \n\n

    For more information, refer to the numpy module and examine the\nmethods and attributes of an array.

    \n\n
    Parameters
    \n\n
      \n
    • (for the __new__ method; see Notes below)
    • \n
    • shape (tuple of ints):\nShape of created array.
    • \n
    • dtype (data-type, optional):\nAny object that can be interpreted as a numpy data type.
    • \n
    • buffer (object exposing buffer interface, optional):\nUsed to fill the array with data.
    • \n
    • offset (int, optional):\nOffset of array data in buffer.
    • \n
    • strides (tuple of ints, optional):\nStrides of data in memory.
    • \n
    • order ({'C', 'F'}, optional):\nRow-major (C-style) or column-major (Fortran-style) order.
    • \n
    \n\n
    Attributes
    \n\n
      \n
    • T (ndarray):\nTranspose of the array.
    • \n
    • data (buffer):\nThe array's elements, in memory.
    • \n
    • dtype (dtype object):\nDescribes the format of the elements in the array.
    • \n
    • flags (dict):\nDictionary containing information related to memory use, e.g.,\n'C_CONTIGUOUS', 'OWNDATA', 'WRITEABLE', etc.
    • \n
    • flat (numpy.flatiter object):\nFlattened version of the array as an iterator. The iterator\nallows assignments, e.g., x.flat = 3 (See ndarray.flat for\nassignment examples; TODO).
    • \n
    • imag (ndarray):\nImaginary part of the array.
    • \n
    • real (ndarray):\nReal part of the array.
    • \n
    • size (int):\nNumber of elements in the array.
    • \n
    • itemsize (int):\nThe memory use of each array element in bytes.
    • \n
    • nbytes (int):\nThe total number of bytes required to store the array data,\ni.e., itemsize * size.
    • \n
    • ndim (int):\nThe array's number of dimensions.
    • \n
    • shape (tuple of ints):\nShape of the array.
    • \n
    • strides (tuple of ints):\nThe step-size required to move from one element to the next in\nmemory. For example, a contiguous (3, 4) array of type\nint16 in C-order has strides (8, 2). This implies that\nto move from element to element in memory requires jumps of 2 bytes.\nTo move from row-to-row, one needs to jump 8 bytes at a time\n(2 * 4).
    • \n
    • ctypes (ctypes object):\nClass containing properties of the array needed for interaction\nwith ctypes.
    • \n
    • base (ndarray):\nIf the array is a view into another array, that array is its base\n(unless that array is also a view). The base array is where the\narray data is actually stored.
    • \n
    \n\n
    See Also
    \n\n

    array: Construct an array.
    \nzeros: Create an array, each element of which is zero.
    \nempty: Create an array, but leave its allocated memory unchanged (i.e.,\nit contains \"garbage\").
    \ndtype: Create a data-type.
    \nnumpy.typing.NDArray: An ndarray alias :term:generic <generic type>\nw.r.t. its dtype.type <numpy.dtype.type>.

    \n\n
    Notes
    \n\n

    There are two modes of creating an array using __new__:

    \n\n
      \n
    1. If buffer is None, then only shape, dtype, and order\nare used.
    2. \n
    3. If buffer is an object exposing the buffer interface, then\nall keywords are interpreted.
    4. \n
    \n\n

    No __init__ method is needed because the array is fully initialized\nafter the __new__ method.

    \n\n
    Examples
    \n\n

    These examples illustrate the low-level ndarray constructor. Refer\nto the See Also section above for easier ways of constructing an\nndarray.

    \n\n

    First mode, buffer is None:

    \n\n
    \n
    >>> np.ndarray(shape=(2,2), dtype=float, order='F')\narray([[0.0e+000, 0.0e+000], # random\n       [     nan, 2.5e-323]])\n
    \n
    \n\n

    Second mode:

    \n\n
    \n
    >>> np.ndarray((2,), buffer=np.array([1,2,3]),\n...            offset=np.int_().itemsize,\n...            dtype=int) # offset = 1*itemsize, i.e. skip first element\narray([2, 3])\n
    \n
    \n", "bases": "numpy.ndarray"}, "pyerrors.input.hadrons.Npr_matrix.g5H": {"fullname": "pyerrors.input.hadrons.Npr_matrix.g5H", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.g5H", "kind": "variable", "doc": "

    Gamma_5 hermitean conjugate

    \n\n

    Uses the fact that the propagator is gamma5 hermitean, so just the\nin and out momenta of the propagator are exchanged.

    \n"}, "pyerrors.input.hadrons.read_ExternalLeg_hd5": {"fullname": "pyerrors.input.hadrons.read_ExternalLeg_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_ExternalLeg_hd5", "kind": "function", "doc": "

    Read hadrons ExternalLeg hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (Npr_matrix):\nread Cobs-matrix
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Bilinear_hd5": {"fullname": "pyerrors.input.hadrons.read_Bilinear_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Bilinear_hd5", "kind": "function", "doc": "

    Read hadrons Bilinear hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result_dict (dict[Npr_matrix]):\nextracted Bilinears
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Fourquark_hd5": {"fullname": "pyerrors.input.hadrons.read_Fourquark_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Fourquark_hd5", "kind": "function", "doc": "

    Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    • vertices (list):\nVertex functions to be extracted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result_dict (dict):\nextracted fourquark matrizes
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None, vertices=['VA', 'AV']):", "funcdef": "def"}, "pyerrors.input.json": {"fullname": "pyerrors.input.json", "modulename": "pyerrors.input.json", "kind": "module", "doc": "

    \n"}, "pyerrors.input.json.create_json_string": {"fullname": "pyerrors.input.json.create_json_string", "modulename": "pyerrors.input.json", "qualname": "create_json_string", "kind": "function", "doc": "

    Generate the string for the export of a list of Obs or structures containing Obs\nto a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • json_string (str):\nString for export to .json(.gz) file
    • \n
    \n", "signature": "(ol, description='', indent=1):", "funcdef": "def"}, "pyerrors.input.json.dump_to_json": {"fullname": "pyerrors.input.json.dump_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_to_json", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    • gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • Null
    • \n
    \n", "signature": "(ol, fname, description='', indent=1, gz=True):", "funcdef": "def"}, "pyerrors.input.json.import_json_string": {"fullname": "pyerrors.input.json.import_json_string", "modulename": "pyerrors.input.json", "qualname": "import_json_string", "kind": "function", "doc": "

    Reconstruct a list of Obs or structures containing Obs from a json string.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.

    \n\n
    Parameters
    \n\n
      \n
    • json_string (str):\njson string containing the data.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nreconstructed list of observables from the json string
    • \n
    • or
    • \n
    • result (Obs):\nonly one observable if the list only has one entry
    • \n
    • or
    • \n
    • result (dict):\nif full_output=True
    • \n
    \n", "signature": "(json_string, verbose=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.load_json": {"fullname": "pyerrors.input.json.load_json", "modulename": "pyerrors.input.json", "qualname": "load_json", "kind": "function", "doc": "

    Import a list of Obs or structures containing Obs from a .json(.gz) file.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nreconstructed list of observables from the json string
    • \n
    • or
    • \n
    • result (Obs):\nonly one observable if the list only has one entry
    • \n
    • or
    • \n
    • result (dict):\nif full_output=True
    • \n
    \n", "signature": "(fname, verbose=True, gz=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.dump_dict_to_json": {"fullname": "pyerrors.input.json.dump_dict_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_dict_to_json", "kind": "function", "doc": "

    Export a dict of Obs or structures containing Obs to a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • od (dict):\nDict of JSON valid structures and objects that will be exported.\nAt the moment, these objects can be either of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    • reps (str):\nSpecify the structure of the placeholder in exported dict to be reps[0-9]+.
    • \n
    • gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(od, fname, description='', indent=1, reps='DICTOBS', gz=True):", "funcdef": "def"}, "pyerrors.input.json.load_json_dict": {"fullname": "pyerrors.input.json.load_json_dict", "modulename": "pyerrors.input.json", "qualname": "load_json_dict", "kind": "function", "doc": "

    Import a dict of Obs or structures containing Obs from a .json(.gz) file.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    • reps (str):\nSpecify the structure of the placeholder in imported dict to be reps[0-9]+.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (Obs / list / Corr):\nRead data
    • \n
    • or
    • \n
    • data (dict):\nRead data and meta-data
    • \n
    \n", "signature": "(fname, verbose=True, gz=True, full_output=False, reps='DICTOBS'):", "funcdef": "def"}, "pyerrors.input.misc": {"fullname": "pyerrors.input.misc", "modulename": "pyerrors.input.misc", "kind": "module", "doc": "

    \n"}, "pyerrors.input.misc.read_pbp": {"fullname": "pyerrors.input.misc.read_pbp", "modulename": "pyerrors.input.misc", "qualname": "read_pbp", "kind": "function", "doc": "

    Read pbp format from given folder structure.

    \n\n
    Parameters
    \n\n
      \n
    • r_start (list):\nlist which contains the first config to be read for each replicum
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nlist of observables read
    • \n
    \n", "signature": "(path, prefix, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD": {"fullname": "pyerrors.input.openQCD", "modulename": "pyerrors.input.openQCD", "kind": "module", "doc": "

    \n"}, "pyerrors.input.openQCD.read_rwms": {"fullname": "pyerrors.input.openQCD.read_rwms", "modulename": "pyerrors.input.openQCD", "qualname": "read_rwms", "kind": "function", "doc": "

    Read rwms format from given folder structure. Returns a list of length nrw

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath that contains the data files
    • \n
    • prefix (str):\nall files in path that start with prefix are considered as input files.\nMay be used together postfix to consider only special file endings.\nPrefix is ignored, if the keyword 'files' is used.
    • \n
    • version (str):\nversion of openQCD, default 2.0
    • \n
    • names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum
    • \n
    • r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.ms1' for openQCD-files
    • \n
    • files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
    • \n
    • print_err (bool):\nPrint additional information that is useful for debugging.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • rwms (Obs):\nReweighting factors read
    • \n
    \n", "signature": "(path, prefix, version='2.0', names=None, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.extract_t0": {"fullname": "pyerrors.input.openQCD.extract_t0", "modulename": "pyerrors.input.openQCD", "qualname": "extract_t0", "kind": "function", "doc": "

    Extract t0 from given .ms.dat files. Returns t0 as Obs.

    \n\n

    It is assumed that all boundary effects have\nsufficiently decayed at x0=xmin.\nThe data around the zero crossing of t^2 - 0.3\nis fitted with a linear function\nfrom which the exact root is extracted.

    \n\n

    It is assumed that one measurement is performed for each config.\nIf this is not the case, the resulting idl, as well as the handling\nof r_start, r_stop and r_step is wrong and the user has to correct\nthis in the resulting observable.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nPath to .ms.dat files
    • \n
    • prefix (str):\nEnsemble prefix
    • \n
    • dtr_read (int):\nDetermines how many trajectories should be skipped\nwhen reading the ms.dat files.\nCorresponds to dtr_cnfg / dtr_ms in the openQCD input file.
    • \n
    • xmin (int):\nFirst timeslice where the boundary\neffects have sufficiently decayed.
    • \n
    • spatial_extent (int):\nspatial extent of the lattice, required for normalization.
    • \n
    • fit_range (int):\nNumber of data points left and right of the zero\ncrossing to be included in the linear fit. (Default: 5)
    • \n
    • postfix (str):\nPostfix of measurement file (Default: ms)
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
    • \n
    • plaquette (bool):\nIf true extract the plaquette estimate of t0 instead.
    • \n
    • names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
    • \n
    • files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
    • \n
    • plot_fit (bool):\nIf true, the fit for the extraction of t0 is shown together with the data.
    • \n
    • assume_thermalization (bool):\nIf True: If the first record divided by the distance between two measurements is larger than\n1, it is assumed that this is due to thermalization and the first measurement belongs\nto the first config (default).\nIf False: The config numbers are assumed to be traj_number // difference
    • \n
    \n\n
    Returns
    \n\n
      \n
    • t0 (Obs):\nExtracted t0
    • \n
    \n", "signature": "(\tpath,\tprefix,\tdtr_read,\txmin,\tspatial_extent,\tfit_range=5,\tpostfix='ms',\t**kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop": {"fullname": "pyerrors.input.openQCD.read_qtop", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop", "kind": "function", "doc": "

    Read the topologial charge based on openQCD gradient flow measurements.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files.
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • version (str):\nEither openQCD or sfqcd, depending on the data.
    • \n
    • L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
    • \n
    • integer_charge (bool):\nIf True, the charge is rounded towards the nearest integer on each config.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (Obs):\nRead topological charge
    • \n
    \n", "signature": "(path, prefix, c, dtr_cnfg=1, version='openQCD', **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_gf_coupling": {"fullname": "pyerrors.input.openQCD.read_gf_coupling", "modulename": "pyerrors.input.openQCD", "qualname": "read_gf_coupling", "kind": "function", "doc": "

    Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.

    \n\n

    Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files.
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
    • \n
    \n", "signature": "(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.qtop_projection": {"fullname": "pyerrors.input.openQCD.qtop_projection", "modulename": "pyerrors.input.openQCD", "qualname": "qtop_projection", "kind": "function", "doc": "

    Returns the projection to the topological charge sector defined by target.

    \n\n
    Parameters
    \n\n
      \n
    • path (Obs):\nTopological charge.
    • \n
    • target (int):\nSpecifies the topological sector to be reweighted to (default 0)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • reto (Obs):\nprojection to the topological charge sector defined by target
    • \n
    \n", "signature": "(qtop, target=0):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop_sector": {"fullname": "pyerrors.input.openQCD.read_qtop_sector", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop_sector", "kind": "function", "doc": "

    Constructs reweighting factors to a specified topological sector.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L
    • \n
    • target (int):\nSpecifies the topological sector to be reweighted to (default 0)
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of trajectories\nbetween two configs.\nif it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • version (str):\nversion string of the openQCD (sfqcd) version used to create\nthe ensemble. Default is 2.0. May also be set to sfqcd.
    • \n
    • L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
    • \n
    • r_start (list):\noffset of the first ensemble, making it easier to match\nlater on with other Obs
    • \n
    • r_stop (list):\nlast configurations that need to be read (per replicum)
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • reto (Obs):\nprojection to the topological charge sector defined by target
    • \n
    \n", "signature": "(path, prefix, c, target=0, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_ms5_xsf": {"fullname": "pyerrors.input.openQCD.read_ms5_xsf", "modulename": "pyerrors.input.openQCD", "qualname": "read_ms5_xsf", "kind": "function", "doc": "

    Read data from files in the specified directory with the specified prefix and quark combination extension, and return a Corr object containing the data.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nThe directory to search for the files in.
    • \n
    • prefix (str):\nThe prefix to match the files against.
    • \n
    • qc (str):\nThe quark combination extension to match the files against.
    • \n
    • corr (str):\nThe correlator to extract data for.
    • \n
    • sep (str, optional):\nThe separator to use when parsing the replika names.
    • \n
    • **kwargs: Additional keyword arguments. The following keyword arguments are recognized:

      \n\n
        \n
      • names (List[str]): A list of names to use for the replicas.
      • \n
    • \n
    \n\n
    Returns
    \n\n
      \n
    • Corr: A complex valued Corr object containing the data read from the files. In case of boudary to bulk correlators.
    • \n
    • or
    • \n
    • CObs: A complex valued CObs object containing the data read from the files. In case of boudary to boundary correlators.
    • \n
    \n\n
    Raises
    \n\n
      \n
    • FileNotFoundError: If no files matching the specified prefix and quark combination extension are found in the specified directory.
    • \n
    • IOError: If there is an error reading a file.
    • \n
    • struct.error: If there is an error unpacking binary data.
    • \n
    \n", "signature": "(path, prefix, qc, corr, sep='r', **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas": {"fullname": "pyerrors.input.pandas", "modulename": "pyerrors.input.pandas", "kind": "module", "doc": "

    \n"}, "pyerrors.input.pandas.to_sql": {"fullname": "pyerrors.input.pandas.to_sql", "modulename": "pyerrors.input.pandas", "qualname": "to_sql", "kind": "function", "doc": "

    Write DataFrame including Obs or Corr valued columns to sqlite database.

    \n\n
    Parameters
    \n\n
      \n
    • df (pandas.DataFrame):\nDataframe to be written to the database.
    • \n
    • table_name (str):\nName of the table in the database.
    • \n
    • db (str):\nPath to the sqlite database.
    • \n
    • if exists (str):\nHow to behave if table already exists. Options 'fail', 'replace', 'append'.
    • \n
    • gz (bool):\nIf True the json strings are gzipped.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(df, table_name, db, if_exists='fail', gz=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.read_sql": {"fullname": "pyerrors.input.pandas.read_sql", "modulename": "pyerrors.input.pandas", "qualname": "read_sql", "kind": "function", "doc": "

    Execute SQL query on sqlite database and obtain DataFrame including Obs or Corr valued columns.

    \n\n
    Parameters
    \n\n
      \n
    • sql (str):\nSQL query to be executed.
    • \n
    • db (str):\nPath to the sqlite database.
    • \n
    • auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (pandas.DataFrame):\nDataframe with the content of the sqlite database.
    • \n
    \n", "signature": "(sql, db, auto_gamma=False, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.dump_df": {"fullname": "pyerrors.input.pandas.dump_df", "modulename": "pyerrors.input.pandas", "qualname": "dump_df", "kind": "function", "doc": "

    Exports a pandas DataFrame containing Obs valued columns to a (gzipped) csv file.

    \n\n

    Before making use of pandas to_csv functionality Obs objects are serialized via the standardized\njson format of pyerrors.

    \n\n
    Parameters
    \n\n
      \n
    • df (pandas.DataFrame):\nDataframe to be dumped to a file.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • gz (bool):\nIf True, the output is a gzipped csv file. If False, the output is a csv file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(df, fname, gz=True):", "funcdef": "def"}, "pyerrors.input.pandas.load_df": {"fullname": "pyerrors.input.pandas.load_df", "modulename": "pyerrors.input.pandas", "qualname": "load_df", "kind": "function", "doc": "

    Imports a pandas DataFrame from a csv.(gz) file in which Obs objects are serialized as json strings.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (pandas.DataFrame):\nDataframe with the content of the sqlite database.
    • \n
    \n", "signature": "(fname, auto_gamma=False, gz=True):", "funcdef": "def"}, "pyerrors.input.sfcf": {"fullname": "pyerrors.input.sfcf", "modulename": "pyerrors.input.sfcf", "kind": "module", "doc": "

    \n"}, "pyerrors.input.sfcf.read_sfcf": {"fullname": "pyerrors.input.sfcf.read_sfcf", "modulename": "pyerrors.input.sfcf", "qualname": "read_sfcf", "kind": "function", "doc": "

    Read sfcf files from given folder structure.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nPath to the sfcf files.
    • \n
    • prefix (str):\nPrefix of the sfcf files.
    • \n
    • name (str):\nName of the correlation function to read.
    • \n
    • quarks (str):\nLabel of the quarks used in the sfcf input file. e.g. \"quark quark\"\nfor version 0.0 this does NOT need to be given with the typical \" - \"\nthat is present in the output file,\nthis is done automatically for this version
    • \n
    • corr_type (str):\nType of correlation function to read. Can be\n
        \n
      • 'bi' for boundary-inner
      • \n
      • 'bb' for boundary-boundary
      • \n
      • 'bib' for boundary-inner-boundary
      • \n
    • \n
    • noffset (int):\nOffset of the source (only relevant when wavefunctions are used)
    • \n
    • wf (int):\nID of wave function
    • \n
    • wf2 (int):\nID of the second wavefunction\n(only relevant for boundary-to-boundary correlation functions)
    • \n
    • im (bool):\nif True, read imaginary instead of real part\nof the correlation function.
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
    • \n
    • ens_name (str):\nreplaces the name of the ensemble
    • \n
    • version (str):\nversion of SFCF, with which the measurement was done.\nif the compact output option (-c) was specified,\nappend a \"c\" to the version (e.g. \"1.0c\")\nif the append output option (-a) was specified,\nappend an \"a\" to the version
    • \n
    • cfg_separator (str):\nString that separates the ensemble identifier from the configuration number (default 'n').
    • \n
    • replica (list):\nlist of replica to be read, default is all
    • \n
    • files (list):\nlist of files to be read per replica, default is all.\nfor non-compact output format, hand the folders to be read here.
    • \n
    • check_configs (list[list[int]]):\nlist of list of supposed configs, eg. [range(1,1000)]\nfor one replicum with 1000 configs
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nlist of Observables with length T, observable per timeslice.\nbb-type correlators have length 1.
    • \n
    \n", "signature": "(\tpath,\tprefix,\tname,\tquarks='.*',\tcorr_type='bi',\tnoffset=0,\twf=0,\twf2=0,\tversion='1.0c',\tcfg_separator='n',\tsilent=False,\t**kwargs):", "funcdef": "def"}, "pyerrors.input.utils": {"fullname": "pyerrors.input.utils", "modulename": "pyerrors.input.utils", "kind": "module", "doc": "

    \n"}, "pyerrors.input.utils.sort_names": {"fullname": "pyerrors.input.utils.sort_names", "modulename": "pyerrors.input.utils", "qualname": "sort_names", "kind": "function", "doc": "

    Sorts a list of names of replika with searches for r and id in the replikum string.\nIf this search fails, a fallback method is used,\nwhere the strings are simply compared and the first diffeing numeral is used for differentiation.

    \n\n
    Parameters
    \n\n
      \n
    • ll (list):\nlist to sort
    • \n
    \n\n
    Returns
    \n\n
      \n
    • ll (list):\nsorted list
    • \n
    \n", "signature": "(ll):", "funcdef": "def"}, "pyerrors.input.utils.check_idl": {"fullname": "pyerrors.input.utils.check_idl", "modulename": "pyerrors.input.utils", "qualname": "check_idl", "kind": "function", "doc": "

    Checks if list of configurations is contained in an idl

    \n\n
    Parameters
    \n\n
      \n
    • idl (range or list):\nidl of the current replicum
    • \n
    • che (list):\nlist of configurations to be checked against
    • \n
    \n\n
    Returns
    \n\n
      \n
    • miss_str (str):\nstring with integers of which idls are missing
    • \n
    \n", "signature": "(idl, che):", "funcdef": "def"}, "pyerrors.linalg": {"fullname": "pyerrors.linalg", "modulename": "pyerrors.linalg", "kind": "module", "doc": "

    \n"}, "pyerrors.linalg.matmul": {"fullname": "pyerrors.linalg.matmul", "modulename": "pyerrors.linalg", "qualname": "matmul", "kind": "function", "doc": "

    Matrix multiply all operands.

    \n\n
    Parameters
    \n\n
      \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    • This implementation is faster compared to standard multiplication via the @ operator.
    • \n
    \n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.jack_matmul": {"fullname": "pyerrors.linalg.jack_matmul", "modulename": "pyerrors.linalg", "qualname": "jack_matmul", "kind": "function", "doc": "

    Matrix multiply both operands making use of the jackknife approximation.

    \n\n
    Parameters
    \n\n
      \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    • For large matrices this is considerably faster compared to matmul.
    • \n
    \n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.einsum": {"fullname": "pyerrors.linalg.einsum", "modulename": "pyerrors.linalg", "qualname": "einsum", "kind": "function", "doc": "

    Wrapper for numpy.einsum

    \n\n
    Parameters
    \n\n
      \n
    • subscripts (str):\nSubscripts for summation (see numpy documentation for details)
    • \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    \n", "signature": "(subscripts, *operands):", "funcdef": "def"}, "pyerrors.linalg.inv": {"fullname": "pyerrors.linalg.inv", "modulename": "pyerrors.linalg", "qualname": "inv", "kind": "function", "doc": "

    Inverse of Obs or CObs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.cholesky": {"fullname": "pyerrors.linalg.cholesky", "modulename": "pyerrors.linalg", "qualname": "cholesky", "kind": "function", "doc": "

    Cholesky decomposition of Obs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.det": {"fullname": "pyerrors.linalg.det", "modulename": "pyerrors.linalg", "qualname": "det", "kind": "function", "doc": "

    Determinant of Obs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.eigh": {"fullname": "pyerrors.linalg.eigh", "modulename": "pyerrors.linalg", "qualname": "eigh", "kind": "function", "doc": "

    Computes the eigenvalues and eigenvectors of a given hermitian matrix of Obs according to np.linalg.eigh.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.eig": {"fullname": "pyerrors.linalg.eig", "modulename": "pyerrors.linalg", "qualname": "eig", "kind": "function", "doc": "

    Computes the eigenvalues of a given matrix of Obs according to np.linalg.eig.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.pinv": {"fullname": "pyerrors.linalg.pinv", "modulename": "pyerrors.linalg", "qualname": "pinv", "kind": "function", "doc": "

    Computes the Moore-Penrose pseudoinverse of a matrix of Obs.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.svd": {"fullname": "pyerrors.linalg.svd", "modulename": "pyerrors.linalg", "qualname": "svd", "kind": "function", "doc": "

    Computes the singular value decomposition of a matrix of Obs.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.misc": {"fullname": "pyerrors.misc", "modulename": "pyerrors.misc", "kind": "module", "doc": "

    \n"}, "pyerrors.misc.print_config": {"fullname": "pyerrors.misc.print_config", "modulename": "pyerrors.misc", "qualname": "print_config", "kind": "function", "doc": "

    Print information about version of python, pyerrors and dependencies.

    \n", "signature": "():", "funcdef": "def"}, "pyerrors.misc.errorbar": {"fullname": "pyerrors.misc.errorbar", "modulename": "pyerrors.misc", "qualname": "errorbar", "kind": "function", "doc": "

    pyerrors wrapper for the errorbars method of matplotlib

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nA list of x-values which can be Obs.
    • \n
    • y (list):\nA list of y-values which can be Obs.
    • \n
    • axes ((matplotlib.pyplot.axes)):\nThe axes to plot on. default is plt.
    • \n
    \n", "signature": "(\tx,\ty,\taxes=<module 'matplotlib.pyplot' from '/opt/hostedtoolcache/Python/3.10.11/x64/lib/python3.10/site-packages/matplotlib/pyplot.py'>,\t**kwargs):", "funcdef": "def"}, "pyerrors.misc.dump_object": {"fullname": "pyerrors.misc.dump_object", "modulename": "pyerrors.misc", "qualname": "dump_object", "kind": "function", "doc": "

    Dump object into pickle file.

    \n\n
    Parameters
    \n\n
      \n
    • obj (object):\nobject to be saved in the pickle file
    • \n
    • name (str):\nname of the file
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(obj, name, **kwargs):", "funcdef": "def"}, "pyerrors.misc.load_object": {"fullname": "pyerrors.misc.load_object", "modulename": "pyerrors.misc", "qualname": "load_object", "kind": "function", "doc": "

    Load object from pickle file.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the file
    • \n
    \n\n
    Returns
    \n\n
      \n
    • object (Obs):\nLoaded Object
    • \n
    \n", "signature": "(path):", "funcdef": "def"}, "pyerrors.misc.pseudo_Obs": {"fullname": "pyerrors.misc.pseudo_Obs", "modulename": "pyerrors.misc", "qualname": "pseudo_Obs", "kind": "function", "doc": "

    Generate an Obs object with given value, dvalue and name for test purposes

    \n\n
    Parameters
    \n\n
      \n
    • value (float):\ncentral value of the Obs to be generated.
    • \n
    • dvalue (float):\nerror of the Obs to be generated.
    • \n
    • name (str):\nname of the ensemble for which the Obs is to be generated.
    • \n
    • samples (int):\nnumber of samples for the Obs (default 1000).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (Obs):\nGenerated Observable
    • \n
    \n", "signature": "(value, dvalue, name, samples=1000):", "funcdef": "def"}, "pyerrors.misc.gen_correlated_data": {"fullname": "pyerrors.misc.gen_correlated_data", "modulename": "pyerrors.misc", "qualname": "gen_correlated_data", "kind": "function", "doc": "

    Generate observables with given covariance and autocorrelation times.

    \n\n
    Parameters
    \n\n
      \n
    • means (list):\nlist containing the mean value of each observable.
    • \n
    • cov (numpy.ndarray):\ncovariance matrix for the data to be generated.
    • \n
    • name (str):\nensemble name for the data to be geneated.
    • \n
    • tau (float or list):\ncan either be a real number or a list with an entry for\nevery dataset.
    • \n
    • samples (int):\nnumber of samples to be generated for each observable.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • corr_obs (list[Obs]):\nGenerated observable list
    • \n
    \n", "signature": "(means, cov, name, tau=0.5, samples=1000):", "funcdef": "def"}, "pyerrors.mpm": {"fullname": "pyerrors.mpm", "modulename": "pyerrors.mpm", "kind": "module", "doc": "

    \n"}, "pyerrors.mpm.matrix_pencil_method": {"fullname": "pyerrors.mpm.matrix_pencil_method", "modulename": "pyerrors.mpm", "qualname": "matrix_pencil_method", "kind": "function", "doc": "

    Matrix pencil method to extract k energy levels from data

    \n\n

    Implementation of the matrix pencil method based on\neq. (2.17) of Y. Hua, T. K. Sarkar, IEEE Trans. Acoust. 38, 814-824 (1990)

    \n\n
    Parameters
    \n\n
      \n
    • data (list):\ncan be a list of Obs for the analysis of a single correlator, or a list of lists\nof Obs if several correlators are to analyzed at once.
    • \n
    • k (int):\nNumber of states to extract (default 1).
    • \n
    • p (int):\nmatrix pencil parameter which filters noise. The optimal value is expected between\nlen(data)/3 and 2*len(data)/3. The computation is more expensive the closer p is\nto len(data)/2 but could possibly suppress more noise (default len(data)//2).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • energy_levels (list[Obs]):\nExtracted energy levels
    • \n
    \n", "signature": "(corrs, k=1, p=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs": {"fullname": "pyerrors.obs", "modulename": "pyerrors.obs", "kind": "module", "doc": "

    \n"}, "pyerrors.obs.Obs": {"fullname": "pyerrors.obs.Obs", "modulename": "pyerrors.obs", "qualname": "Obs", "kind": "class", "doc": "

    Class for a general observable.

    \n\n

    Instances of Obs are the basic objects of a pyerrors error analysis.\nThey are initialized with a list which contains arrays of samples for\ndifferent ensembles/replica and another list of same length which contains\nthe names of the ensembles/replica. Mathematical operations can be\nperformed on instances. The result is another instance of Obs. The error of\nan instance can be computed with the gamma_method. Also contains additional\nmethods for output and visualization of the error calculation.

    \n\n
    Attributes
    \n\n
      \n
    • S_global (float):\nStandard value for S (default 2.0)
    • \n
    • S_dict (dict):\nDictionary for S values. If an entry for a given ensemble\nexists this overwrites the standard value for that ensemble.
    • \n
    • tau_exp_global (float):\nStandard value for tau_exp (default 0.0)
    • \n
    • tau_exp_dict (dict):\nDictionary for tau_exp values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
    • \n
    • N_sigma_global (float):\nStandard value for N_sigma (default 1.0)
    • \n
    • N_sigma_dict (dict):\nDictionary for N_sigma values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
    • \n
    \n"}, "pyerrors.obs.Obs.__init__": {"fullname": "pyerrors.obs.Obs.__init__", "modulename": "pyerrors.obs", "qualname": "Obs.__init__", "kind": "function", "doc": "

    Initialize Obs object.

    \n\n
    Parameters
    \n\n
      \n
    • samples (list):\nlist of numpy arrays containing the Monte Carlo samples
    • \n
    • names (list):\nlist of strings labeling the individual samples
    • \n
    • idl (list, optional):\nlist of ranges or lists on which the samples are defined
    • \n
    \n", "signature": "(samples, names, idl=None, **kwargs)"}, "pyerrors.obs.Obs.gamma_method": {"fullname": "pyerrors.obs.Obs.gamma_method", "modulename": "pyerrors.obs", "qualname": "Obs.gamma_method", "kind": "function", "doc": "

    Estimate the error and related properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
    • \n
    • tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
    • \n
    • N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
    • \n
    • fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
    • \n
    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.gm": {"fullname": "pyerrors.obs.Obs.gm", "modulename": "pyerrors.obs", "qualname": "Obs.gm", "kind": "function", "doc": "

    Estimate the error and related properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
    • \n
    • tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
    • \n
    • N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
    • \n
    • fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
    • \n
    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.details": {"fullname": "pyerrors.obs.Obs.details", "modulename": "pyerrors.obs", "qualname": "Obs.details", "kind": "function", "doc": "

    Output detailed properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • ens_content (bool):\nprint details about the ensembles and replica if true.
    • \n
    \n", "signature": "(self, ens_content=True):", "funcdef": "def"}, "pyerrors.obs.Obs.reweight": {"fullname": "pyerrors.obs.Obs.reweight", "modulename": "pyerrors.obs", "qualname": "Obs.reweight", "kind": "function", "doc": "

    Reweight the obs with given rewighting factors.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
    • \n
    \n", "signature": "(self, weight):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero_within_error": {"fullname": "pyerrors.obs.Obs.is_zero_within_error", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero_within_error", "kind": "function", "doc": "

    Checks whether the observable is zero within 'sigma' standard errors.

    \n\n
    Parameters
    \n\n
      \n
    • sigma (int):\nNumber of standard errors used for the check.
    • \n
    • Works only properly when the gamma method was run.
    • \n
    \n", "signature": "(self, sigma=1):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero": {"fullname": "pyerrors.obs.Obs.is_zero", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero", "kind": "function", "doc": "

    Checks whether the observable is zero within a given tolerance.

    \n\n
    Parameters
    \n\n
      \n
    • atol (float):\nAbsolute tolerance (for details see numpy documentation).
    • \n
    \n", "signature": "(self, atol=1e-10):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_tauint": {"fullname": "pyerrors.obs.Obs.plot_tauint", "modulename": "pyerrors.obs", "qualname": "Obs.plot_tauint", "kind": "function", "doc": "

    Plot integrated autocorrelation time for each ensemble.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rho": {"fullname": "pyerrors.obs.Obs.plot_rho", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rho", "kind": "function", "doc": "

    Plot normalized autocorrelation function time for each ensemble.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rep_dist": {"fullname": "pyerrors.obs.Obs.plot_rep_dist", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rep_dist", "kind": "function", "doc": "

    Plot replica distribution for each ensemble with more than one replicum.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_history": {"fullname": "pyerrors.obs.Obs.plot_history", "modulename": "pyerrors.obs", "qualname": "Obs.plot_history", "kind": "function", "doc": "

    Plot derived Monte Carlo history for each ensemble

    \n\n
    Parameters
    \n\n
      \n
    • expand (bool):\nshow expanded history for irregular Monte Carlo chains (default: True).
    • \n
    \n", "signature": "(self, expand=True):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_piechart": {"fullname": "pyerrors.obs.Obs.plot_piechart", "modulename": "pyerrors.obs", "qualname": "Obs.plot_piechart", "kind": "function", "doc": "

    Plot piechart which shows the fractional contribution of each\nensemble to the error and returns a dictionary containing the fractions.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.dump": {"fullname": "pyerrors.obs.Obs.dump", "modulename": "pyerrors.obs", "qualname": "Obs.dump", "kind": "function", "doc": "

    Dump the Obs to a file 'name' of chosen format.

    \n\n
    Parameters
    \n\n
      \n
    • filename (str):\nname of the file to be saved.
    • \n
    • datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
    • \n
    • description (str):\nDescription for output file, only relevant for json.gz format.
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n", "signature": "(self, filename, datatype='json.gz', description='', **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.export_jackknife": {"fullname": "pyerrors.obs.Obs.export_jackknife", "modulename": "pyerrors.obs", "qualname": "Obs.export_jackknife", "kind": "function", "doc": "

    Export jackknife samples from the Obs

    \n\n
    Returns
    \n\n
      \n
    • numpy.ndarray: Returns a numpy array of length N + 1 where N is the number of samples\nfor the given ensemble and replicum. The zeroth entry of the array contains\nthe mean value of the Obs, entries 1 to N contain the N jackknife samples\nderived from the Obs. The current implementation only works for observables\ndefined on exactly one ensemble and replicum. The derived jackknife samples\nshould agree with samples from a full jackknife analysis up to O(1/N).
    • \n
    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sqrt": {"fullname": "pyerrors.obs.Obs.sqrt", "modulename": "pyerrors.obs", "qualname": "Obs.sqrt", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.log": {"fullname": "pyerrors.obs.Obs.log", "modulename": "pyerrors.obs", "qualname": "Obs.log", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.exp": {"fullname": "pyerrors.obs.Obs.exp", "modulename": "pyerrors.obs", "qualname": "Obs.exp", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sin": {"fullname": "pyerrors.obs.Obs.sin", "modulename": "pyerrors.obs", "qualname": "Obs.sin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cos": {"fullname": "pyerrors.obs.Obs.cos", "modulename": "pyerrors.obs", "qualname": "Obs.cos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tan": {"fullname": "pyerrors.obs.Obs.tan", "modulename": "pyerrors.obs", "qualname": "Obs.tan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsin": {"fullname": "pyerrors.obs.Obs.arcsin", "modulename": "pyerrors.obs", "qualname": "Obs.arcsin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccos": {"fullname": "pyerrors.obs.Obs.arccos", "modulename": "pyerrors.obs", "qualname": "Obs.arccos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctan": {"fullname": "pyerrors.obs.Obs.arctan", "modulename": "pyerrors.obs", "qualname": "Obs.arctan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sinh": {"fullname": "pyerrors.obs.Obs.sinh", "modulename": "pyerrors.obs", "qualname": "Obs.sinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cosh": {"fullname": "pyerrors.obs.Obs.cosh", "modulename": "pyerrors.obs", "qualname": "Obs.cosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tanh": {"fullname": "pyerrors.obs.Obs.tanh", "modulename": "pyerrors.obs", "qualname": "Obs.tanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsinh": {"fullname": "pyerrors.obs.Obs.arcsinh", "modulename": "pyerrors.obs", "qualname": "Obs.arcsinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccosh": {"fullname": "pyerrors.obs.Obs.arccosh", "modulename": "pyerrors.obs", "qualname": "Obs.arccosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctanh": {"fullname": "pyerrors.obs.Obs.arctanh", "modulename": "pyerrors.obs", "qualname": "Obs.arctanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs": {"fullname": "pyerrors.obs.CObs", "modulename": "pyerrors.obs", "qualname": "CObs", "kind": "class", "doc": "

    Class for a complex valued observable.

    \n"}, "pyerrors.obs.CObs.__init__": {"fullname": "pyerrors.obs.CObs.__init__", "modulename": "pyerrors.obs", "qualname": "CObs.__init__", "kind": "function", "doc": "

    \n", "signature": "(real, imag=0.0)"}, "pyerrors.obs.CObs.gamma_method": {"fullname": "pyerrors.obs.CObs.gamma_method", "modulename": "pyerrors.obs", "qualname": "CObs.gamma_method", "kind": "function", "doc": "

    Executes the gamma_method for the real and the imaginary part.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.CObs.is_zero": {"fullname": "pyerrors.obs.CObs.is_zero", "modulename": "pyerrors.obs", "qualname": "CObs.is_zero", "kind": "function", "doc": "

    Checks whether both real and imaginary part are zero within machine precision.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs.conjugate": {"fullname": "pyerrors.obs.CObs.conjugate", "modulename": "pyerrors.obs", "qualname": "CObs.conjugate", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.derived_observable": {"fullname": "pyerrors.obs.derived_observable", "modulename": "pyerrors.obs", "qualname": "derived_observable", "kind": "function", "doc": "

    Construct a derived Obs according to func(data, **kwargs) using automatic differentiation.

    \n\n
    Parameters
    \n\n
      \n
    • func (object):\narbitrary function of the form func(data, **kwargs). For the\nautomatic differentiation to work, all numpy functions have to have\nthe autograd wrapper (use 'import autograd.numpy as anp').
    • \n
    • data (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
    • \n
    • num_grad (bool):\nif True, numerical derivatives are used instead of autograd\n(default False). To control the numerical differentiation the\nkwargs of numdifftools.step_generators.MaxStepGenerator\ncan be used.
    • \n
    • man_grad (list):\nmanually supply a list or an array which contains the jacobian\nof func. Use cautiously, supplying the wrong derivative will\nnot be intercepted.
    • \n
    \n\n
    Notes
    \n\n

    For simple mathematical operations it can be practical to use anonymous\nfunctions. For the ratio of two observables one can e.g. use

    \n\n

    new_obs = derived_observable(lambda x: x[0] / x[1], [obs1, obs2])

    \n", "signature": "(func, data, array_mode=False, **kwargs):", "funcdef": "def"}, "pyerrors.obs.reweight": {"fullname": "pyerrors.obs.reweight", "modulename": "pyerrors.obs", "qualname": "reweight", "kind": "function", "doc": "

    Reweight a list of observables.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • obs (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
    • \n
    \n", "signature": "(weight, obs, **kwargs):", "funcdef": "def"}, "pyerrors.obs.correlate": {"fullname": "pyerrors.obs.correlate", "modulename": "pyerrors.obs", "qualname": "correlate", "kind": "function", "doc": "

    Correlate two observables.

    \n\n
    Parameters
    \n\n
      \n
    • obs_a (Obs):\nFirst observable
    • \n
    • obs_b (Obs):\nSecond observable
    • \n
    \n\n
    Notes
    \n\n

    Keep in mind to only correlate primary observables which have not been reweighted\nyet. The reweighting has to be applied after correlating the observables.\nCurrently only works if ensembles are identical (this is not strictly necessary).

    \n", "signature": "(obs_a, obs_b):", "funcdef": "def"}, "pyerrors.obs.covariance": {"fullname": "pyerrors.obs.covariance", "modulename": "pyerrors.obs", "qualname": "covariance", "kind": "function", "doc": "

    Calculates the error covariance matrix of a set of observables.

    \n\n

    WARNING: This function should be used with care, especially for observables with support on multiple\n ensembles with differing autocorrelations. See the notes below for details.

    \n\n

    The gamma method has to be applied first to all observables.

    \n\n
    Parameters
    \n\n
      \n
    • obs (list or numpy.ndarray):\nList or one dimensional array of Obs
    • \n
    • visualize (bool):\nIf True plots the corresponding normalized correlation matrix (default False).
    • \n
    • correlation (bool):\nIf True the correlation matrix instead of the error covariance matrix is returned (default False).
    • \n
    • smooth (None or int):\nIf smooth is an integer 'E' between 2 and the dimension of the matrix minus 1 the eigenvalue\nsmoothing procedure of hep-lat/9412087 is applied to the correlation matrix which leaves the\nlargest E eigenvalues essentially unchanged and smoothes the smaller eigenvalues to avoid extremely\nsmall ones.
    • \n
    \n\n
    Notes
    \n\n

    The error covariance is defined such that it agrees with the squared standard error for two identical observables\n$$\\operatorname{cov}(a,a)=\\sum_{s=1}^N\\delta_a^s\\delta_a^s/N^2=\\Gamma_{aa}(0)/N=\\operatorname{var}(a)/N=\\sigma_a^2$$\nin the absence of autocorrelation.\nThe error covariance is estimated by calculating the correlation matrix assuming no autocorrelation and then rescaling the correlation matrix by the full errors including the previous gamma method estimate for the autocorrelation of the observables. The covariance at windowsize 0 is guaranteed to be positive semi-definite\n$$\\sum_{i,j}v_i\\Gamma_{ij}(0)v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i,j}v_i\\delta_i^s\\delta_j^s v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i}|v_i\\delta_i^s|^2\\geq 0\\,,$$ for every $v\\in\\mathbb{R}^M$, while such an identity does not hold for larger windows/lags.\nFor observables defined on a single ensemble our approximation is equivalent to assuming that the integrated autocorrelation time of an off-diagonal element is equal to the geometric mean of the integrated autocorrelation times of the corresponding diagonal elements.\n$$\\tau_{\\mathrm{int}, ij}=\\sqrt{\\tau_{\\mathrm{int}, i}\\times \\tau_{\\mathrm{int}, j}}$$\nThis construction ensures that the estimated covariance matrix is positive semi-definite (up to numerical rounding errors).

    \n", "signature": "(obs, visualize=False, correlation=False, smooth=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs.import_jackknife": {"fullname": "pyerrors.obs.import_jackknife", "modulename": "pyerrors.obs", "qualname": "import_jackknife", "kind": "function", "doc": "

    Imports jackknife samples and returns an Obs

    \n\n
    Parameters
    \n\n
      \n
    • jacks (numpy.ndarray):\nnumpy array containing the mean value as zeroth entry and\nthe N jackknife samples as first to Nth entry.
    • \n
    • name (str):\nname of the ensemble the samples are defined on.
    • \n
    \n", "signature": "(jacks, name, idl=None):", "funcdef": "def"}, "pyerrors.obs.merge_obs": {"fullname": "pyerrors.obs.merge_obs", "modulename": "pyerrors.obs", "qualname": "merge_obs", "kind": "function", "doc": "

    Combine all observables in list_of_obs into one new observable

    \n\n
    Parameters
    \n\n
      \n
    • list_of_obs (list):\nlist of the Obs object to be combined
    • \n
    \n\n
    Notes
    \n\n

    It is not possible to combine obs which are based on the same replicum

    \n", "signature": "(list_of_obs):", "funcdef": "def"}, "pyerrors.obs.cov_Obs": {"fullname": "pyerrors.obs.cov_Obs", "modulename": "pyerrors.obs", "qualname": "cov_Obs", "kind": "function", "doc": "

    Create an Obs based on mean(s) and a covariance matrix

    \n\n
    Parameters
    \n\n
      \n
    • mean (list of floats or float):\nN mean value(s) of the new Obs
    • \n
    • cov (list or array):\n2d (NxN) Covariance matrix, 1d diagonal entries or 0d covariance
    • \n
    • name (str):\nidentifier for the covariance matrix
    • \n
    • grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
    • \n
    \n", "signature": "(means, cov, name, grad=None):", "funcdef": "def"}, "pyerrors.roots": {"fullname": "pyerrors.roots", "modulename": "pyerrors.roots", "kind": "module", "doc": "

    \n"}, "pyerrors.roots.find_root": {"fullname": "pyerrors.roots.find_root", "modulename": "pyerrors.roots", "qualname": "find_root", "kind": "function", "doc": "

    Finds the root of the function func(x, d) where d is an Obs.

    \n\n
    Parameters
    \n\n
      \n
    • d (Obs):\nObs passed to the function.
    • \n
    • func (object):\nFunction to be minimized. Any numpy functions have to use the autograd.numpy wrapper.\nExample:

      \n\n
      \n
      import autograd.numpy as anp\ndef root_func(x, d):\n   return anp.exp(-x ** 2) - d\n
      \n
    • \n
    • guess (float):\nInitial guess for the minimization.

    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (Obs):\nObs valued root of the function.
    • \n
    \n", "signature": "(d, func, guess=1.0, **kwargs):", "funcdef": "def"}, "pyerrors.version": {"fullname": "pyerrors.version", "modulename": "pyerrors.version", "kind": "module", "doc": "

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    What is pyerrors?

    \n\n

    pyerrors is a python package for error computation and propagation of Markov chain Monte Carlo data.\nIt is based on the gamma method arXiv:hep-lat/0306017. Some of its features are:

    \n\n
      \n
    • automatic differentiation for exact linear error propagation as suggested in arXiv:1809.01289 (partly based on the autograd package).
    • \n
    • treatment of slow modes in the simulation as suggested in arXiv:1009.5228.
    • \n
    • coherent error propagation for data from different Markov chains.
    • \n
    • non-linear fits with x- and y-errors and exact linear error propagation based on automatic differentiation as introduced in arXiv:1809.01289.
    • \n
    • real and complex matrix operations and their error propagation based on automatic differentiation (Matrix inverse, Cholesky decomposition, calculation of eigenvalues and eigenvectors, singular value decomposition...).
    • \n
    \n\n

    More detailed examples can found in the GitHub repository \"badge\".

    \n\n

    If you use pyerrors for research that leads to a publication please consider citing:

    \n\n
      \n
    • Fabian Joswig, Simon Kuberski, Justus T. Kuhlmann, Jan Neuendorf, pyerrors: a python framework for error analysis of Monte Carlo data. [arXiv:2209.14371 [hep-lat]].
    • \n
    • Ulli Wolff, Monte Carlo errors with less errors. Comput.Phys.Commun. 156 (2004) 143-153, Comput.Phys.Commun. 176 (2007) 383 (erratum).
    • \n
    • Alberto Ramos, Automatic differentiation for error analysis of Monte Carlo data. Comput.Phys.Commun. 238 (2019) 19-35.
    • \n
    \n\n

    and

    \n\n
      \n
    • Stefan Schaefer, Rainer Sommer, Francesco Virotta, Critical slowing down and error analysis in lattice QCD simulations. Nucl.Phys.B 845 (2011) 93-119.
    • \n
    \n\n

    where applicable.

    \n\n

    There exist similar publicly available implementations of gamma method error analysis suites in Fortran, Julia and Python.

    \n\n

    Installation

    \n\n

    Install the most recent release using pip and pypi:

    \n\n
    \n
    pip install pyerrors     # Fresh install\npip install -U pyerrors  # Update\n
    \n
    \n\n

    Install the most recent release using conda and conda-forge:

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    \n
    conda install -c conda-forge pyerrors  # Fresh install\nconda update -c conda-forge pyerrors   # Update\n
    \n
    \n\n

    Install the current develop version:

    \n\n
    \n
    pip install git+https://github.com/fjosw/pyerrors.git@develop\n
    \n
    \n\n

    Basic example

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    \n
    import numpy as np\nimport pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name']) # Initialize an Obs object\nmy_new_obs = 2 * np.log(my_obs) / my_obs ** 2 # Construct derived Obs object\nmy_new_obs.gamma_method()                     # Estimate the statistical error\nprint(my_new_obs)                             # Print the result to stdout\n> 0.31498(72)\n
    \n
    \n\n

    The Obs class

    \n\n

    pyerrors introduces a new datatype, Obs, which simplifies error propagation and estimation for auto- and cross-correlated data.\nAn Obs object can be initialized with two arguments, the first is a list containing the samples for an observable from a Monte Carlo chain.\nThe samples can either be provided as python list or as numpy array.\nThe second argument is a list containing the names of the respective Monte Carlo chains as strings. These strings uniquely identify a Monte Carlo chain/ensemble. It is crucial for the correct error propagation that observations from the same Monte Carlo history are labeled with the same name. See Multiple ensembles/replica for details.

    \n\n
    \n
    import pyerrors as pe\n\nmy_obs = pe.Obs([samples], ['ensemble_name'])\n
    \n
    \n\n

    Error propagation

    \n\n

    When performing mathematical operations on Obs objects the correct error propagation is intrinsically taken care of using a first order Taylor expansion\n$$\\delta_f^i=\\sum_\\alpha \\bar{f}_\\alpha \\delta_\\alpha^i\\,,\\quad \\delta_\\alpha^i=a_\\alpha^i-\\bar{a}_\\alpha\\,,$$\nas introduced in arXiv:hep-lat/0306017.\nThe required derivatives $\\bar{f}_\\alpha$ are evaluated up to machine precision via automatic differentiation as suggested in arXiv:1809.01289.

    \n\n

    The Obs class is designed such that mathematical numpy functions can be used on Obs just as for regular floats.

    \n\n
    \n
    import numpy as np\nimport pyerrors as pe\n\nmy_obs1 = pe.Obs([samples1], ['ensemble_name'])\nmy_obs2 = pe.Obs([samples2], ['ensemble_name'])\n\nmy_sum = my_obs1 + my_obs2\n\nmy_m_eff = np.log(my_obs1 / my_obs2)\n\niamzero = my_m_eff - my_m_eff\n# Check that value and fluctuations are zero within machine precision\nprint(iamzero == 0.0)\n> True\n
    \n
    \n\n

    Error estimation

    \n\n

    The error estimation within pyerrors is based on the gamma method introduced in arXiv:hep-lat/0306017.\nAfter having arrived at the derived quantity of interest the gamma_method can be called as detailed in the following example.

    \n\n
    \n
    my_sum.gamma_method()\nprint(my_sum)\n> 1.70(57)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 5.72046658e-01 +/- 7.56746598e-02 (33.650%)\n>  t_int         2.71422900e+00 +/- 6.40320983e-01 S = 2.00\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    We use the following definition of the integrated autocorrelation time established in Madras & Sokal 1988\n$$\\tau_\\mathrm{int}=\\frac{1}{2}+\\sum_{t=1}^{W}\\rho(t)\\geq \\frac{1}{2}\\,.$$\nThe window $W$ is determined via the automatic windowing procedure described in arXiv:hep-lat/0306017.\nThe standard value for the parameter $S$ of this automatic windowing procedure is $S=2$. Other values for $S$ can be passed to the gamma_method as parameter.

    \n\n
    \n
    my_sum.gamma_method(S=3.0)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 6.30675201e-01 +/- 1.04585650e-01 (37.099%)\n>  t_int         3.29909703e+00 +/- 9.77310102e-01 S = 3.00\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    The integrated autocorrelation time $\\tau_\\mathrm{int}$ and the autocorrelation function $\\rho(W)$ can be monitored via the methods pyerrors.obs.Obs.plot_tauint and pyerrors.obs.Obs.plot_rho.

    \n\n

    If the parameter $S$ is set to zero it is assumed that the dataset does not exhibit any autocorrelation and the window size is chosen to be zero.\nIn this case the error estimate is identical to the sample standard error.

    \n\n

    Exponential tails

    \n\n

    Slow modes in the Monte Carlo history can be accounted for by attaching an exponential tail to the autocorrelation function $\\rho$ as suggested in arXiv:1009.5228. The longest autocorrelation time in the history, $\\tau_\\mathrm{exp}$, can be passed to the gamma_method as parameter. In this case the automatic windowing procedure is vacated and the parameter $S$ does not affect the error estimate.

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    \n
    my_sum.gamma_method(tau_exp=7.2)\nmy_sum.details()\n> Result         1.70000000e+00 +/- 6.28097762e-01 +/- 5.79077524e-02 (36.947%)\n>  t_int         3.27218667e+00 +/- 7.99583654e-01 tau_exp = 7.20,  N_sigma = 1\n> 1000 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble_name' : 1000 configurations (from 1 to 1000)\n
    \n
    \n\n

    For the full API see pyerrors.obs.Obs.gamma_method.

    \n\n

    Multiple ensembles/replica

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    Error propagation for multiple ensembles (Markov chains with different simulation parameters) is handled automatically. Ensembles are uniquely identified by their name.

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    \n
    obs1 = pe.Obs([samples1], ['ensemble1'])\nobs2 = pe.Obs([samples2], ['ensemble2'])\n\nmy_sum = obs1 + obs2\nmy_sum.details()\n> Result   2.00697958e+00\n> 1500 samples in 2 ensembles:\n>   \u00b7 Ensemble 'ensemble1' : 1000 configurations (from 1 to 1000)\n>   \u00b7 Ensemble 'ensemble2' : 500 configurations (from 1 to 500)\n
    \n
    \n\n

    Observables from the same Monte Carlo chain have to be initialized with the same name for correct error propagation. If different names were used in this case the data would be treated as statistically independent resulting in loss of relevant information and a potential over or under estimate of the statistical error.

    \n\n

    pyerrors identifies multiple replica (independent Markov chains with identical simulation parameters) by the vertical bar | in the name of the data set.

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    \n
    obs1 = pe.Obs([samples1], ['ensemble1|r01'])\nobs2 = pe.Obs([samples2], ['ensemble1|r02'])\n\n> my_sum = obs1 + obs2\n> my_sum.details()\n> Result   2.00697958e+00\n> 1500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1'\n>     \u00b7 Replicum 'r01' : 1000 configurations (from 1 to 1000)\n>     \u00b7 Replicum 'r02' : 500 configurations (from 1 to 500)\n
    \n
    \n\n

    Error estimation for multiple ensembles

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    In order to keep track of different error analysis parameters for different ensembles one can make use of global dictionaries as detailed in the following example.

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    \n
    pe.Obs.S_dict['ensemble1'] = 2.5\npe.Obs.tau_exp_dict['ensemble2'] = 8.0\npe.Obs.tau_exp_dict['ensemble3'] = 2.0\n
    \n
    \n\n

    In case the gamma_method is called without any parameters it will use the values specified in the dictionaries for the respective ensembles.\nPassing arguments to the gamma_method still dominates over the dictionaries.

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    Irregular Monte Carlo chains

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    Obs objects defined on irregular Monte Carlo chains can be initialized with the parameter idl.

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    \n
    # Observable defined on configurations 20 to 519\nobs1 = pe.Obs([samples1], ['ensemble1'], idl=[range(20, 520)])\nobs1.details()\n> Result         9.98319881e-01\n> 500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 500 configurations (from 20 to 519)\n\n# Observable defined on every second configuration between 5 and 1003\nobs2 = pe.Obs([samples2], ['ensemble1'], idl=[range(5, 1005, 2)])\nobs2.details()\n> Result         9.99100712e-01\n> 500 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 500 configurations (from 5 to 1003 in steps of 2)\n\n# Observable defined on configurations 2, 9, 28, 29 and 501\nobs3 = pe.Obs([samples3], ['ensemble1'], idl=[[2, 9, 28, 29, 501]])\nobs3.details()\n> Result         1.01718064e+00\n> 5 samples in 1 ensemble:\n>   \u00b7 Ensemble 'ensemble1' : 5 configurations (irregular range)\n
    \n
    \n\n

    Obs objects defined on regular and irregular histories of the same ensemble can be combined with each other and the correct error propagation and estimation is automatically taken care of.

    \n\n

    Warning: Irregular Monte Carlo chains can result in odd patterns in the autocorrelation functions.\nMake sure to check the autocorrelation time with e.g. pyerrors.obs.Obs.plot_rho or pyerrors.obs.Obs.plot_tauint.

    \n\n

    For the full API see pyerrors.obs.Obs.

    \n\n

    Correlators

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    When one is not interested in single observables but correlation functions, pyerrors offers the Corr class which simplifies the corresponding error propagation and provides the user with a set of standard methods. In order to initialize a Corr objects one needs to arrange the data as a list of Obs

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    \n
    my_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3])\nprint(my_corr)\n> x0/a  Corr(x0/a)\n> ------------------\n> 0      0.7957(80)\n> 1      0.5156(51)\n> 2      0.3227(33)\n> 3      0.2041(21)\n
    \n
    \n\n

    In case the correlation functions are not defined on the outermost timeslices, for example because of fixed boundary conditions, a padding can be introduced.

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    \n
    my_corr = pe.Corr([obs_0, obs_1, obs_2, obs_3], padding=[1, 1])\nprint(my_corr)\n> x0/a  Corr(x0/a)\n> ------------------\n> 0\n> 1      0.7957(80)\n> 2      0.5156(51)\n> 3      0.3227(33)\n> 4      0.2041(21)\n> 5\n
    \n
    \n\n

    The individual entries of a correlator can be accessed via slicing

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    print(my_corr[3])\n> 0.3227(33)\n
    \n
    \n\n

    Error propagation with the Corr class works very similar to Obs objects. Mathematical operations are overloaded and Corr objects can be computed together with other Corr objects, Obs objects or real numbers and integers.

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    \n
    my_new_corr = 0.3 * my_corr[2] * my_corr * my_corr + 12 / my_corr\n
    \n
    \n\n

    pyerrors provides the user with a set of regularly used methods for the manipulation of correlator objects:

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      \n
    • Corr.gamma_method applies the gamma method to all entries of the correlator.
    • \n
    • Corr.m_eff to construct effective masses. Various variants for periodic and fixed temporal boundary conditions are available.
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    • Corr.deriv returns the first derivative of the correlator as Corr. Different discretizations of the numerical derivative are available.
    • \n
    • Corr.second_deriv returns the second derivative of the correlator as Corr. Different discretizations of the numerical derivative are available.
    • \n
    • Corr.symmetric symmetrizes parity even correlations functions, assuming periodic boundary conditions.
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    • Corr.anti_symmetric anti-symmetrizes parity odd correlations functions, assuming periodic boundary conditions.
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    • Corr.T_symmetry averages a correlator with its time symmetry partner, assuming fixed boundary conditions.
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    • Corr.plateau extracts a plateau value from the correlator in a given range.
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    • Corr.roll periodically shifts the correlator.
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    • Corr.reverse reverses the time ordering of the correlator.
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    • Corr.correlate constructs a disconnected correlation function from the correlator and another Corr or Obs object.
    • \n
    • Corr.reweight reweights the correlator.
    • \n
    \n\n

    pyerrors can also handle matrices of correlation functions and extract energy states from these matrices via a generalized eigenvalue problem (see pyerrors.correlators.Corr.GEVP).

    \n\n

    For the full API see pyerrors.correlators.Corr.

    \n\n

    Complex valued observables

    \n\n

    pyerrors can handle complex valued observables via the class pyerrors.obs.CObs.\nCObs are initialized with a real and an imaginary part which both can be Obs valued.

    \n\n
    \n
    my_real_part = pe.Obs([samples1], ['ensemble1'])\nmy_imag_part = pe.Obs([samples2], ['ensemble1'])\n\nmy_cobs = pe.CObs(my_real_part, my_imag_part)\nmy_cobs.gamma_method()\nprint(my_cobs)\n> (0.9959(91)+0.659(28)j)\n
    \n
    \n\n

    Elementary mathematical operations are overloaded and samples are properly propagated as for the Obs class.

    \n\n
    \n
    my_derived_cobs = (my_cobs + my_cobs.conjugate()) / np.abs(my_cobs)\nmy_derived_cobs.gamma_method()\nprint(my_derived_cobs)\n> (1.668(23)+0.0j)\n
    \n
    \n\n

    The Covobs class

    \n\n

    In many projects, auxiliary data that is not based on Monte Carlo chains enters. Examples are experimentally determined mesons masses which are used to set the scale or renormalization constants. These numbers come with an error that has to be propagated through the analysis. The Covobs class allows to define such quantities in pyerrors. Furthermore, external input might consist of correlated quantities. An example are the parameters of an interpolation formula, which are defined via mean values and a covariance matrix between all parameters. The contribution of the interpolation formula to the error of a derived quantity therefore might depend on the complete covariance matrix.

    \n\n

    This concept is built into the definition of Covobs. In pyerrors, external input is defined by $M$ mean values, a $M\\times M$ covariance matrix, where $M=1$ is permissible, and a name that uniquely identifies the covariance matrix. Below, we define the pion mass, based on its mean value and error, 134.9768(5). Note, that the square of the error enters cov_Obs, since the second argument of this function is the covariance matrix of the Covobs.

    \n\n
    \n
    import pyerrors.obs as pe\n\nmpi = pe.cov_Obs(134.9768, 0.0005**2, 'pi^0 mass')\nmpi.gamma_method()\nmpi.details()\n> Result         1.34976800e+02 +/- 5.00000000e-04 +/- 0.00000000e+00 (0.000%)\n>  pi^0 mass     5.00000000e-04\n> 0 samples in 1 ensemble:\n>   \u00b7 Covobs   'pi^0 mass'\n
    \n
    \n\n

    The resulting object mpi is an Obs that contains a Covobs. In the following, it may be handled as any other Obs. The contribution of the covariance matrix to the error of an Obs is determined from the $M \\times M$ covariance matrix $\\Sigma$ and the gradient of the Obs with respect to the external quantities, which is the $1\\times M$ Jacobian matrix $J$, via\n$$s = \\sqrt{J^T \\Sigma J}\\,,$$\nwhere the Jacobian is computed for each derived quantity via automatic differentiation.

    \n\n

    Correlated auxiliary data is defined similarly to above, e.g., via

    \n\n
    \n
    RAP = pe.cov_Obs([16.7457, -19.0475], [[3.49591, -6.07560], [-6.07560, 10.5834]], 'R_AP, 1906.03445, (5.3a)')\nprint(RAP)\n> [Obs[16.7(1.9)], Obs[-19.0(3.3)]]\n
    \n
    \n\n

    where RAP now is a list of two Obs that contains the two correlated parameters.

    \n\n

    Since the gradient of a derived observable with respect to an external covariance matrix is propagated through the entire analysis, the Covobs class allows to quote the derivative of a result with respect to the external quantities. If these derivatives are published together with the result, small shifts in the definition of external quantities, e.g., the definition of the physical point, can be performed a posteriori based on the published information. This may help to compare results of different groups. The gradient of an Obs o with respect to a covariance matrix with the identifying string k may be accessed via

    \n\n
    \n
    o.covobs[k].grad\n
    \n
    \n\n

    Error propagation in iterative algorithms

    \n\n

    pyerrors supports exact linear error propagation for iterative algorithms like various variants of non-linear least squares fits or root finding. The derivatives required for the error propagation are calculated as described in arXiv:1809.01289.

    \n\n

    Least squares fits

    \n\n

    Standard non-linear least square fits with errors on the dependent but not the independent variables can be performed with pyerrors.fits.least_squares. As default solver the Levenberg-Marquardt algorithm implemented in scipy is used.

    \n\n

    Fit functions have to be of the following form

    \n\n
    \n
    import autograd.numpy as anp\n\ndef func(a, x):\n    return a[1] * anp.exp(-a[0] * x)\n
    \n
    \n\n

    It is important that numerical functions refer to autograd.numpy instead of numpy for the automatic differentiation in iterative algorithms to work properly.

    \n\n

    Fits can then be performed via

    \n\n
    \n
    fit_result = pe.fits.least_squares(x, y, func)\nprint("\\n", fit_result)\n> Fit with 2 parameters\n> Method: Levenberg-Marquardt\n> `ftol` termination condition is satisfied.\n> chisquare/d.o.f.: 0.9593035785160936\n\n>  Goodness of fit:\n> \u03c7\u00b2/d.o.f. = 0.959304\n> p-value   = 0.5673\n> Fit parameters:\n> 0      0.0548(28)\n> 1      1.933(64)\n
    \n
    \n\n

    where x is a list or numpy.array of floats and y is a list or numpy.array of Obs.

    \n\n

    Data stored in Corr objects can be fitted directly using the Corr.fit method.

    \n\n
    \n
    my_corr = pe.Corr(y)\nfit_result = my_corr.fit(func, fitrange=[12, 25])\n
    \n
    \n\n

    this can simplify working with absolute fit ranges and takes care of gaps in the data automatically.

    \n\n

    For fit functions with multiple independent variables the fit function can be of the form

    \n\n
    \n
    def func(a, x):\n    (x1, x2) = x\n    return a[0] * x1 ** 2 + a[1] * x2\n
    \n
    \n\n

    pyerrors also supports correlated fits which can be triggered via the parameter correlated_fit=True.\nDetails about how the required covariance matrix is estimated can be found in pyerrors.obs.covariance.

    \n\n

    Direct visualizations of the performed fits can be triggered via resplot=True or qqplot=True. For all available options see pyerrors.fits.least_squares.

    \n\n

    Total least squares fits

    \n\n

    pyerrors can also fit data with errors on both the dependent and independent variables using the total least squares method also referred to orthogonal distance regression as implemented in scipy, see pyerrors.fits.least_squares. The syntax is identical to the standard least squares case, the only difference being that x also has to be a list or numpy.array of Obs.

    \n\n

    For the full API see pyerrors.fits for fits and pyerrors.roots for finding roots of functions.

    \n\n

    Matrix operations

    \n\n

    pyerrors provides wrappers for Obs- and CObs-valued matrix operations based on numpy.linalg. The supported functions include:

    \n\n
      \n
    • inv for the matrix inverse.
    • \n
    • cholseky for the Cholesky decomposition.
    • \n
    • det for the matrix determinant.
    • \n
    • eigh for eigenvalues and eigenvectors of hermitean matrices.
    • \n
    • eig for eigenvalues of general matrices.
    • \n
    • pinv for the Moore-Penrose pseudoinverse.
    • \n
    • svd for the singular-value-decomposition.
    • \n
    \n\n

    For the full API see pyerrors.linalg.

    \n\n

    Export data

    \n\n

    \n\n

    The preferred exported file format within pyerrors is json.gz. Files written to this format are valid JSON files that have been compressed using gzip. The structure of the content is inspired by the dobs format of the ALPHA collaboration. The aim of the format is to facilitate the storage of data in a self-contained way such that, even years after the creation of the file, it is possible to extract all necessary information:

    \n\n
      \n
    • What observables are stored? Possibly: How exactly are they defined.
    • \n
    • How does each single ensemble or external quantity contribute to the error of the observable?
    • \n
    • Who did write the file when and on which machine?
    • \n
    \n\n

    This can be achieved by storing all information in one single file. The export routines of pyerrors are written such that as much information as possible is written automatically as described in the following example

    \n\n
    \n
    my_obs = pe.Obs([samples], ["test_ensemble"])\nmy_obs.tag = "My observable"\n\npe.input.json.dump_to_json(my_obs, "test_output_file", description="This file contains a test observable")\n# For a single observable one can equivalently use the class method dump\nmy_obs.dump("test_output_file", description="This file contains a test observable")\n\ncheck = pe.input.json.load_json("test_output_file")\n\nprint(my_obs == check)\n> True\n
    \n
    \n\n

    The format also allows to directly write out the content of Corr objects or lists and arrays of Obs objects by passing the desired data to pyerrors.input.json.dump_to_json.

    \n\n

    json.gz format specification

    \n\n

    The first entries of the file provide optional auxiliary information:

    \n\n
      \n
    • program is a string that indicates which program was used to write the file.
    • \n
    • version is a string that specifies the version of the format.
    • \n
    • who is a string that specifies the user name of the creator of the file.
    • \n
    • date is a string and contains the creation date of the file.
    • \n
    • host is a string and contains the hostname of the machine where the file has been written.
    • \n
    • description contains information on the content of the file. This field is not filled automatically in pyerrors. The user is advised to provide as detailed information as possible in this field. Examples are: Input files of measurements or simulations, LaTeX formulae or references to publications to specify how the observables have been computed, details on the analysis strategy, ... This field may be any valid JSON type. Strings, arrays or objects (equivalent to dicts in python) are well suited to provide information.
    • \n
    \n\n

    The only necessary entry of the file is the field\n-obsdata, an array that contains the actual data.

    \n\n

    Each entry of the array belongs to a single structure of observables. Currently, these structures can be either of Obs, list, numpy.ndarray, Corr. All Obs inside a structure (with dimension > 0) have to be defined on the same set of configurations. Different structures, that are represented by entries of the array obsdata, are treated independently. Each entry of the array obsdata has the following required entries:

    \n\n
      \n
    • type is a string that specifies the type of the structure. This allows to parse the content to the correct form after reading the file. It is always possible to interpret the content as list of Obs.
    • \n
    • value is an array that contains the mean values of the Obs inside the structure.\nThe following entries are optional:
    • \n
    • layout is a string that specifies the layout of multi-dimensional structures. Examples are \"2, 2\" for a 2x2 dimensional matrix or \"64, 4, 4\" for a Corr with $T=64$ and 4x4 matrices on each time slices. \"1\" denotes a single Obs. Multi-dimensional structures are stored in row-major format (see below).
    • \n
    • tag is any JSON type. It contains additional information concerning the structure. The tag of an Obs in pyerrors is written here.
    • \n
    • reweighted is a Bool that may be used to specify, whether the Obs in the structure have been reweighted.
    • \n
    • data is an array that contains the data from MC chains. We will define it below.
    • \n
    • cdata is an array that contains the data from external quantities with an error (Covobs in pyerrors). We will define it below.
    • \n
    \n\n

    The array data contains the data from MC chains. Each entry of the array corresponds to one ensemble and contains:

    \n\n
      \n
    • id, a string that contains the name of the ensemble
    • \n
    • replica, an array that contains an entry per replica of the ensemble.
    • \n
    \n\n

    Each entry of replica contains\nname, a string that contains the name of the replica\ndeltas, an array that contains the actual data.

    \n\n

    Each entry in deltas corresponds to one configuration of the replica and has $1+N$ many entries. The first entry is an integer that specifies the configuration number that, together with ensemble and replica name, may be used to uniquely identify the configuration on which the data has been obtained. The following N entries specify the deltas, i.e., the deviation of the observable from the mean value on this configuration, of each Obs inside the structure. Multi-dimensional structures are stored in a row-major format. For primary observables, such as correlation functions, $value + delta_i$ matches the primary data obtained on the configuration.

    \n\n

    The array cdata contains information about the contribution of auxiliary observables, represented by Covobs in pyerrors, to the total error of the observables. Each entry of the array belongs to one auxiliary covariance matrix and contains:

    \n\n
      \n
    • id, a string that identifies the covariance matrix
    • \n
    • layout, a string that defines the dimensions of the $M\\times M$ covariance matrix (has to be \"M, M\" or \"1\").
    • \n
    • cov, an array that contains the $M\\times M$ many entries of the covariance matrix, stored in row-major format.
    • \n
    • grad, an array that contains N entries, one for each Obs inside the structure. Each entry itself is an array, that contains the M gradients of the Nth observable with respect to the quantity that corresponds to the Mth diagonal entry of the covariance matrix.
    • \n
    \n\n

    A JSON schema that may be used to verify the correctness of a file with respect to the format definition is stored in ./examples/json_schema.json. The schema is a self-descriptive format definition and contains an exemplary file.

    \n\n

    Julia I/O routines for the json.gz format, compatible with ADerrors.jl, can be found here.

    \n"}, "pyerrors.correlators": {"fullname": "pyerrors.correlators", "modulename": "pyerrors.correlators", "kind": "module", "doc": "

    \n"}, "pyerrors.correlators.Corr": {"fullname": "pyerrors.correlators.Corr", "modulename": "pyerrors.correlators", "qualname": "Corr", "kind": "class", "doc": "

    The class for a correlator (time dependent sequence of pe.Obs).

    \n\n

    Everything, this class does, can be achieved using lists or arrays of Obs.\nBut it is simply more convenient to have a dedicated object for correlators.\nOne often wants to add or multiply correlators of the same length at every timeslice and it is inconvenient\nto iterate over all timeslices for every operation. This is especially true, when dealing with matrices.

    \n\n

    The correlator can have two types of content: An Obs at every timeslice OR a GEVP\nmatrix at every timeslice. Other dependency (eg. spatial) are not supported.

    \n"}, "pyerrors.correlators.Corr.__init__": {"fullname": "pyerrors.correlators.Corr.__init__", "modulename": "pyerrors.correlators", "qualname": "Corr.__init__", "kind": "function", "doc": "

    Initialize a Corr object.

    \n\n
    Parameters
    \n\n
      \n
    • data_input (list or array):\nlist of Obs or list of arrays of Obs or array of Corrs
    • \n
    • padding (list, optional):\nList with two entries where the first labels the padding\nat the front of the correlator and the second the padding\nat the back.
    • \n
    • prange (list, optional):\nList containing the first and last timeslice of the plateau\nregion indentified for this correlator.
    • \n
    \n", "signature": "(data_input, padding=[0, 0], prange=None)"}, "pyerrors.correlators.Corr.gamma_method": {"fullname": "pyerrors.correlators.Corr.gamma_method", "modulename": "pyerrors.correlators", "qualname": "Corr.gamma_method", "kind": "function", "doc": "

    Apply the gamma method to the content of the Corr.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.gm": {"fullname": "pyerrors.correlators.Corr.gm", "modulename": "pyerrors.correlators", "qualname": "Corr.gm", "kind": "function", "doc": "

    Apply the gamma method to the content of the Corr.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.projected": {"fullname": "pyerrors.correlators.Corr.projected", "modulename": "pyerrors.correlators", "qualname": "Corr.projected", "kind": "function", "doc": "

    We need to project the Correlator with a Vector to get a single value at each timeslice.

    \n\n

    The method can use one or two vectors.\nIf two are specified it returns v1@G@v2 (the order might be very important.)\nBy default it will return the lowest source, which usually means unsmeared-unsmeared (0,0), but it does not have to

    \n", "signature": "(self, vector_l=None, vector_r=None, normalize=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.item": {"fullname": "pyerrors.correlators.Corr.item", "modulename": "pyerrors.correlators", "qualname": "Corr.item", "kind": "function", "doc": "

    Picks the element [i,j] from every matrix and returns a correlator containing one Obs per timeslice.

    \n\n
    Parameters
    \n\n
      \n
    • i (int):\nFirst index to be picked.
    • \n
    • j (int):\nSecond index to be picked.
    • \n
    \n", "signature": "(self, i, j):", "funcdef": "def"}, "pyerrors.correlators.Corr.plottable": {"fullname": "pyerrors.correlators.Corr.plottable", "modulename": "pyerrors.correlators", "qualname": "Corr.plottable", "kind": "function", "doc": "

    Outputs the correlator in a plotable format.

    \n\n

    Outputs three lists containing the timeslice index, the value on each\ntimeslice and the error on each timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.symmetric": {"fullname": "pyerrors.correlators.Corr.symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.symmetric", "kind": "function", "doc": "

    Symmetrize the correlator around x0=0.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.anti_symmetric": {"fullname": "pyerrors.correlators.Corr.anti_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.anti_symmetric", "kind": "function", "doc": "

    Anti-symmetrize the correlator around x0=0.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.is_matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.is_matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.is_matrix_symmetric", "kind": "function", "doc": "

    Checks whether a correlator matrices is symmetric on every timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.matrix_symmetric": {"fullname": "pyerrors.correlators.Corr.matrix_symmetric", "modulename": "pyerrors.correlators", "qualname": "Corr.matrix_symmetric", "kind": "function", "doc": "

    Symmetrizes the correlator matrices on every timeslice.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.GEVP": {"fullname": "pyerrors.correlators.Corr.GEVP", "modulename": "pyerrors.correlators", "qualname": "Corr.GEVP", "kind": "function", "doc": "

    Solve the generalized eigenvalue problem on the correlator matrix and returns the corresponding eigenvectors.

    \n\n

    The eigenvectors are sorted according to the descending eigenvalues, the zeroth eigenvector(s) correspond to the\nlargest eigenvalue(s). The eigenvector(s) for the individual states can be accessed via slicing

    \n\n
    \n
    C.GEVP(t0=2)[0]  # Ground state vector(s)\nC.GEVP(t0=2)[:3]  # Vectors for the lowest three states\n
    \n
    \n\n
    Parameters
    \n\n
      \n
    • t0 (int):\nThe time t0 for the right hand side of the GEVP according to $G(t)v_i=\\lambda_i G(t_0)v_i$
    • \n
    • ts (int):\nfixed time $G(t_s)v_i=\\lambda_i G(t_0)v_i$ if sort=None.\nIf sort=\"Eigenvector\" it gives a reference point for the sorting method.
    • \n
    • sort (string):\nIf this argument is set, a list of self.T vectors per state is returned. If it is set to None, only one vector is returned.\n
        \n
      • \"Eigenvalue\": The eigenvector is chosen according to which eigenvalue it belongs individually on every timeslice.
      • \n
      • \"Eigenvector\": Use the method described in arXiv:2004.10472 to find the set of v(t) belonging to the state.\nThe reference state is identified by its eigenvalue at $t=t_s$.
      • \n
    • \n
    \n\n
    Other Parameters
    \n\n
      \n
    • state (int):\nReturns only the vector(s) for a specified state. The lowest state is zero.
    • \n
    \n", "signature": "(self, t0, ts=None, sort='Eigenvalue', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.Eigenvalue": {"fullname": "pyerrors.correlators.Corr.Eigenvalue", "modulename": "pyerrors.correlators", "qualname": "Corr.Eigenvalue", "kind": "function", "doc": "

    Determines the eigenvalue of the GEVP by solving and projecting the correlator

    \n\n
    Parameters
    \n\n
      \n
    • state (int):\nThe state one is interested in ordered by energy. The lowest state is zero.
    • \n
    • All other parameters are identical to the ones of Corr.GEVP.
    • \n
    \n", "signature": "(self, t0, ts=None, state=0, sort='Eigenvalue'):", "funcdef": "def"}, "pyerrors.correlators.Corr.Hankel": {"fullname": "pyerrors.correlators.Corr.Hankel", "modulename": "pyerrors.correlators", "qualname": "Corr.Hankel", "kind": "function", "doc": "

    Constructs an NxN Hankel matrix

    \n\n

    C(t) c(t+1) ... c(t+n-1)\nC(t+1) c(t+2) ... c(t+n)\n.................\nC(t+(n-1)) c(t+n) ... c(t+2(n-1))

    \n\n
    Parameters
    \n\n
      \n
    • N (int):\nDimension of the Hankel matrix
    • \n
    • periodic (bool, optional):\ndetermines whether the matrix is extended periodically
    • \n
    \n", "signature": "(self, N, periodic=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.roll": {"fullname": "pyerrors.correlators.Corr.roll", "modulename": "pyerrors.correlators", "qualname": "Corr.roll", "kind": "function", "doc": "

    Periodically shift the correlator by dt timeslices

    \n\n
    Parameters
    \n\n
      \n
    • dt (int):\nnumber of timeslices
    • \n
    \n", "signature": "(self, dt):", "funcdef": "def"}, "pyerrors.correlators.Corr.reverse": {"fullname": "pyerrors.correlators.Corr.reverse", "modulename": "pyerrors.correlators", "qualname": "Corr.reverse", "kind": "function", "doc": "

    Reverse the time ordering of the Corr

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.thin": {"fullname": "pyerrors.correlators.Corr.thin", "modulename": "pyerrors.correlators", "qualname": "Corr.thin", "kind": "function", "doc": "

    Thin out a correlator to suppress correlations

    \n\n
    Parameters
    \n\n
      \n
    • spacing (int):\nKeep only every 'spacing'th entry of the correlator
    • \n
    • offset (int):\nOffset the equal spacing
    • \n
    \n", "signature": "(self, spacing=2, offset=0):", "funcdef": "def"}, "pyerrors.correlators.Corr.correlate": {"fullname": "pyerrors.correlators.Corr.correlate", "modulename": "pyerrors.correlators", "qualname": "Corr.correlate", "kind": "function", "doc": "

    Correlate the correlator with another correlator or Obs

    \n\n
    Parameters
    \n\n
      \n
    • partner (Obs or Corr):\npartner to correlate the correlator with.\nCan either be an Obs which is correlated with all entries of the\ncorrelator or a Corr of same length.
    • \n
    \n", "signature": "(self, partner):", "funcdef": "def"}, "pyerrors.correlators.Corr.reweight": {"fullname": "pyerrors.correlators.Corr.reweight", "modulename": "pyerrors.correlators", "qualname": "Corr.reweight", "kind": "function", "doc": "

    Reweight the correlator.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl.
    • \n
    \n", "signature": "(self, weight, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.T_symmetry": {"fullname": "pyerrors.correlators.Corr.T_symmetry", "modulename": "pyerrors.correlators", "qualname": "Corr.T_symmetry", "kind": "function", "doc": "

    Return the time symmetry average of the correlator and its partner

    \n\n
    Parameters
    \n\n
      \n
    • partner (Corr):\nTime symmetry partner of the Corr
    • \n
    • partity (int):\nParity quantum number of the correlator, can be +1 or -1
    • \n
    \n", "signature": "(self, partner, parity=1):", "funcdef": "def"}, "pyerrors.correlators.Corr.deriv": {"fullname": "pyerrors.correlators.Corr.deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.deriv", "kind": "function", "doc": "

    Return the first derivative of the correlator with respect to x0.

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, forward, backward, improved, log, default: symmetric
    • \n
    \n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.second_deriv": {"fullname": "pyerrors.correlators.Corr.second_deriv", "modulename": "pyerrors.correlators", "qualname": "Corr.second_deriv", "kind": "function", "doc": "

    Return the second derivative of the correlator with respect to x0.

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\ndecides which definition of the finite differences derivative is used.\nAvailable choice: symmetric, improved, log, default: symmetric
    • \n
    \n", "signature": "(self, variant='symmetric'):", "funcdef": "def"}, "pyerrors.correlators.Corr.m_eff": {"fullname": "pyerrors.correlators.Corr.m_eff", "modulename": "pyerrors.correlators", "qualname": "Corr.m_eff", "kind": "function", "doc": "

    Returns the effective mass of the correlator as correlator object

    \n\n
    Parameters
    \n\n
      \n
    • variant (str):\nlog : uses the standard effective mass log(C(t) / C(t+1))\ncosh, periodic : Use periodicitiy of the correlator by solving C(t) / C(t+1) = cosh(m * (t - T/2)) / cosh(m * (t + 1 - T/2)) for m.\nsinh : Use anti-periodicitiy of the correlator by solving C(t) / C(t+1) = sinh(m * (t - T/2)) / sinh(m * (t + 1 - T/2)) for m.\nSee, e.g., arXiv:1205.5380\narccosh : Uses the explicit form of the symmetrized correlator (not recommended)\nlogsym: uses the symmetric effective mass log(C(t-1) / C(t+1))/2
    • \n
    • guess (float):\nguess for the root finder, only relevant for the root variant
    • \n
    \n", "signature": "(self, variant='log', guess=1.0):", "funcdef": "def"}, "pyerrors.correlators.Corr.fit": {"fullname": "pyerrors.correlators.Corr.fit", "modulename": "pyerrors.correlators", "qualname": "Corr.fit", "kind": "function", "doc": "

    Fits function to the data

    \n\n
    Parameters
    \n\n
      \n
    • function (obj):\nfunction to fit to the data. See fits.least_squares for details.
    • \n
    • fitrange (list):\nTwo element list containing the timeslices on which the fit is supposed to start and stop.\nCaution: This range is inclusive as opposed to standard python indexing.\nfitrange=[4, 6] corresponds to the three entries 4, 5 and 6.\nIf not specified, self.prange or all timeslices are used.
    • \n
    • silent (bool):\nDecides whether output is printed to the standard output.
    • \n
    \n", "signature": "(self, function, fitrange=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.plateau": {"fullname": "pyerrors.correlators.Corr.plateau", "modulename": "pyerrors.correlators", "qualname": "Corr.plateau", "kind": "function", "doc": "

    Extract a plateau value from a Corr object

    \n\n
    Parameters
    \n\n
      \n
    • plateau_range (list):\nlist with two entries, indicating the first and the last timeslice\nof the plateau region.
    • \n
    • method (str):\nmethod to extract the plateau.\n 'fit' fits a constant to the plateau region\n 'avg', 'average' or 'mean' just average over the given timeslices.
    • \n
    • auto_gamma (bool):\napply gamma_method with default parameters to the Corr. Defaults to None
    • \n
    \n", "signature": "(self, plateau_range=None, method='fit', auto_gamma=False):", "funcdef": "def"}, "pyerrors.correlators.Corr.set_prange": {"fullname": "pyerrors.correlators.Corr.set_prange", "modulename": "pyerrors.correlators", "qualname": "Corr.set_prange", "kind": "function", "doc": "

    Sets the attribute prange of the Corr object.

    \n", "signature": "(self, prange):", "funcdef": "def"}, "pyerrors.correlators.Corr.show": {"fullname": "pyerrors.correlators.Corr.show", "modulename": "pyerrors.correlators", "qualname": "Corr.show", "kind": "function", "doc": "

    Plots the correlator using the tag of the correlator as label if available.

    \n\n
    Parameters
    \n\n
      \n
    • x_range (list):\nlist of two values, determining the range of the x-axis e.g. [4, 8].
    • \n
    • comp (Corr or list of Corr):\nCorrelator or list of correlators which are plotted for comparison.\nThe tags of these correlators are used as labels if available.
    • \n
    • logscale (bool):\nSets y-axis to logscale.
    • \n
    • plateau (Obs):\nPlateau value to be visualized in the figure.
    • \n
    • fit_res (Fit_result):\nFit_result object to be visualized.
    • \n
    • fit_key (str):\nKey for the fit function in Fit_result.fit_function (for combined fits).
    • \n
    • ylabel (str):\nLabel for the y-axis.
    • \n
    • save (str):\npath to file in which the figure should be saved.
    • \n
    • auto_gamma (bool):\nApply the gamma method with standard parameters to all correlators and plateau values before plotting.
    • \n
    • hide_sigma (float):\nHides data points from the first value on which is consistent with zero within 'hide_sigma' standard errors.
    • \n
    • references (list):\nList of floating point values that are displayed as horizontal lines for reference.
    • \n
    • title (string):\nOptional title of the figure.
    • \n
    \n", "signature": "(\tself,\tx_range=None,\tcomp=None,\ty_range=None,\tlogscale=False,\tplateau=None,\tfit_res=None,\tfit_key=None,\tylabel=None,\tsave=None,\tauto_gamma=False,\thide_sigma=None,\treferences=None,\ttitle=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.spaghetti_plot": {"fullname": "pyerrors.correlators.Corr.spaghetti_plot", "modulename": "pyerrors.correlators", "qualname": "Corr.spaghetti_plot", "kind": "function", "doc": "

    Produces a spaghetti plot of the correlator suited to monitor exceptional configurations.

    \n\n
    Parameters
    \n\n
      \n
    • logscale (bool):\nDetermines whether the scale of the y-axis is logarithmic or standard.
    • \n
    \n", "signature": "(self, logscale=True):", "funcdef": "def"}, "pyerrors.correlators.Corr.dump": {"fullname": "pyerrors.correlators.Corr.dump", "modulename": "pyerrors.correlators", "qualname": "Corr.dump", "kind": "function", "doc": "

    Dumps the Corr into a file of chosen type

    \n\n
    Parameters
    \n\n
      \n
    • filename (str):\nName of the file to be saved.
    • \n
    • datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n", "signature": "(self, filename, datatype='json.gz', **kwargs):", "funcdef": "def"}, "pyerrors.correlators.Corr.print": {"fullname": "pyerrors.correlators.Corr.print", "modulename": "pyerrors.correlators", "qualname": "Corr.print", "kind": "function", "doc": "

    \n", "signature": "(self, print_range=None):", "funcdef": "def"}, "pyerrors.correlators.Corr.sqrt": {"fullname": "pyerrors.correlators.Corr.sqrt", "modulename": "pyerrors.correlators", "qualname": "Corr.sqrt", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.log": {"fullname": "pyerrors.correlators.Corr.log", "modulename": "pyerrors.correlators", "qualname": "Corr.log", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.exp": {"fullname": "pyerrors.correlators.Corr.exp", "modulename": "pyerrors.correlators", "qualname": "Corr.exp", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sin": {"fullname": "pyerrors.correlators.Corr.sin", "modulename": "pyerrors.correlators", "qualname": "Corr.sin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cos": {"fullname": "pyerrors.correlators.Corr.cos", "modulename": "pyerrors.correlators", "qualname": "Corr.cos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tan": {"fullname": "pyerrors.correlators.Corr.tan", "modulename": "pyerrors.correlators", "qualname": "Corr.tan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.sinh": {"fullname": "pyerrors.correlators.Corr.sinh", "modulename": "pyerrors.correlators", "qualname": "Corr.sinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.cosh": {"fullname": "pyerrors.correlators.Corr.cosh", "modulename": "pyerrors.correlators", "qualname": "Corr.cosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.tanh": {"fullname": "pyerrors.correlators.Corr.tanh", "modulename": "pyerrors.correlators", "qualname": "Corr.tanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsin": {"fullname": "pyerrors.correlators.Corr.arcsin", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccos": {"fullname": "pyerrors.correlators.Corr.arccos", "modulename": "pyerrors.correlators", "qualname": "Corr.arccos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctan": {"fullname": "pyerrors.correlators.Corr.arctan", "modulename": "pyerrors.correlators", "qualname": "Corr.arctan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arcsinh": {"fullname": "pyerrors.correlators.Corr.arcsinh", "modulename": "pyerrors.correlators", "qualname": "Corr.arcsinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arccosh": {"fullname": "pyerrors.correlators.Corr.arccosh", "modulename": "pyerrors.correlators", "qualname": "Corr.arccosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.arctanh": {"fullname": "pyerrors.correlators.Corr.arctanh", "modulename": "pyerrors.correlators", "qualname": "Corr.arctanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.correlators.Corr.prune": {"fullname": "pyerrors.correlators.Corr.prune", "modulename": "pyerrors.correlators", "qualname": "Corr.prune", "kind": "function", "doc": "

    Project large correlation matrix to lowest states

    \n\n

    This method can be used to reduce the size of an (N x N) correlation matrix\nto (Ntrunc x Ntrunc) by solving a GEVP at very early times where the noise\nis still small.

    \n\n
    Parameters
    \n\n
      \n
    • Ntrunc (int):\nRank of the target matrix.
    • \n
    • tproj (int):\nTime where the eigenvectors are evaluated, corresponds to ts in the GEVP method.\nThe default value is 3.
    • \n
    • t0proj (int):\nTime where the correlation matrix is inverted. Choosing t0proj=1 is strongly\ndiscouraged for O(a) improved theories, since the correctness of the procedure\ncannot be granted in this case. The default value is 2.
    • \n
    • basematrix (Corr):\nCorrelation matrix that is used to determine the eigenvectors of the\nlowest states based on a GEVP. basematrix is taken to be the Corr itself if\nis is not specified.
    • \n
    \n\n
    Notes
    \n\n

    We have the basematrix $C(t)$ and the target matrix $G(t)$. We start by solving\nthe GEVP $$C(t) v_n(t, t_0) = \\lambda_n(t, t_0) C(t_0) v_n(t, t_0)$$ where $t \\equiv t_\\mathrm{proj}$\nand $t_0 \\equiv t_{0, \\mathrm{proj}}$. The target matrix is projected onto the subspace of the\nresulting eigenvectors $v_n, n=1,\\dots,N_\\mathrm{trunc}$ via\n$$G^\\prime_{i, j}(t) = (v_i, G(t) v_j)$$. This allows to reduce the size of a large\ncorrelation matrix and to remove some noise that is added by irrelevant operators.\nThis may allow to use the GEVP on $G(t)$ at late times such that the theoretically motivated\nbound $t_0 \\leq t/2$ holds, since the condition number of $G(t)$ is decreased, compared to $C(t)$.

    \n", "signature": "(self, Ntrunc, tproj=3, t0proj=2, basematrix=None):", "funcdef": "def"}, "pyerrors.covobs": {"fullname": "pyerrors.covobs", "modulename": "pyerrors.covobs", "kind": "module", "doc": "

    \n"}, "pyerrors.covobs.Covobs": {"fullname": "pyerrors.covobs.Covobs", "modulename": "pyerrors.covobs", "qualname": "Covobs", "kind": "class", "doc": "

    \n"}, "pyerrors.covobs.Covobs.__init__": {"fullname": "pyerrors.covobs.Covobs.__init__", "modulename": "pyerrors.covobs", "qualname": "Covobs.__init__", "kind": "function", "doc": "

    Initialize Covobs object.

    \n\n
    Parameters
    \n\n
      \n
    • mean (float):\nMean value of the new Obs
    • \n
    • cov (list or array):\n2d Covariance matrix or 1d diagonal entries
    • \n
    • name (str):\nidentifier for the covariance matrix
    • \n
    • pos (int):\nPosition of the variance belonging to mean in cov.\nIs taken to be 1 if cov is 0-dimensional
    • \n
    • grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
    • \n
    \n", "signature": "(mean, cov, name, pos=None, grad=None)"}, "pyerrors.covobs.Covobs.errsq": {"fullname": "pyerrors.covobs.Covobs.errsq", "modulename": "pyerrors.covobs", "qualname": "Covobs.errsq", "kind": "function", "doc": "

    Return the variance (= square of the error) of the Covobs

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.dirac": {"fullname": "pyerrors.dirac", "modulename": "pyerrors.dirac", "kind": "module", "doc": "

    \n"}, "pyerrors.dirac.epsilon_tensor": {"fullname": "pyerrors.dirac.epsilon_tensor", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor", "kind": "function", "doc": "

    Rank-3 epsilon tensor

    \n\n

    Based on https://codegolf.stackexchange.com/a/160375

    \n\n
    Returns
    \n\n
      \n
    • elem (int):\nElement (i,j,k) of the epsilon tensor of rank 3
    • \n
    \n", "signature": "(i, j, k):", "funcdef": "def"}, "pyerrors.dirac.epsilon_tensor_rank4": {"fullname": "pyerrors.dirac.epsilon_tensor_rank4", "modulename": "pyerrors.dirac", "qualname": "epsilon_tensor_rank4", "kind": "function", "doc": "

    Rank-4 epsilon tensor

    \n\n

    Extension of https://codegolf.stackexchange.com/a/160375

    \n\n
    Returns
    \n\n
      \n
    • elem (int):\nElement (i,j,k,o) of the epsilon tensor of rank 4
    • \n
    \n", "signature": "(i, j, k, o):", "funcdef": "def"}, "pyerrors.dirac.Grid_gamma": {"fullname": "pyerrors.dirac.Grid_gamma", "modulename": "pyerrors.dirac", "qualname": "Grid_gamma", "kind": "function", "doc": "

    Returns gamma matrix in Grid labeling.

    \n", "signature": "(gamma_tag):", "funcdef": "def"}, "pyerrors.fits": {"fullname": "pyerrors.fits", "modulename": "pyerrors.fits", "kind": "module", "doc": "

    \n"}, "pyerrors.fits.Fit_result": {"fullname": "pyerrors.fits.Fit_result", "modulename": "pyerrors.fits", "qualname": "Fit_result", "kind": "class", "doc": "

    Represents fit results.

    \n\n
    Attributes
    \n\n
      \n
    • fit_parameters (list):\nresults for the individual fit parameters,\nalso accessible via indices.
    • \n
    • chisquare_by_dof (float):\nreduced chisquare.
    • \n
    • p_value (float):\np-value of the fit
    • \n
    • t2_p_value (float):\nHotelling t-squared p-value for correlated fits.
    • \n
    \n", "bases": "collections.abc.Sequence"}, "pyerrors.fits.Fit_result.gamma_method": {"fullname": "pyerrors.fits.Fit_result.gamma_method", "modulename": "pyerrors.fits", "qualname": "Fit_result.gamma_method", "kind": "function", "doc": "

    Apply the gamma method to all fit parameters

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.Fit_result.gm": {"fullname": "pyerrors.fits.Fit_result.gm", "modulename": "pyerrors.fits", "qualname": "Fit_result.gm", "kind": "function", "doc": "

    Apply the gamma method to all fit parameters

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.fits.least_squares": {"fullname": "pyerrors.fits.least_squares", "modulename": "pyerrors.fits", "qualname": "least_squares", "kind": "function", "doc": "

    Performs a non-linear fit to y = func(x).\n ```

    \n\n
    Parameters
    \n\n
      \n
    • For an uncombined fit:
    • \n
    • x (list):\nlist of floats.
    • \n
    • y (list):\nlist of Obs.
    • \n
    • func (object):\nfit function, has to be of the form

      \n\n
      \n
      import autograd.numpy as anp\n\ndef func(a, x):\n   return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
      \n
      \n\n

      For multiple x values func can be of the form

      \n\n
      \n
      def func(a, x):\n   (x1, x2) = x\n   return a[0] * x1 ** 2 + a[1] * x2\n
      \n
      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • OR For a combined fit:
    • \n
    • x (dict):\ndict of lists.
    • \n
    • y (dict):\ndict of lists of Obs.
    • \n
    • funcs (dict):\ndict of objects\nfit functions have to be of the form (here a[0] is the common fit parameter)\n```python\nimport autograd.numpy as anp\nfuncs = {\"a\": func_a,\n \"b\": func_b}

      \n\n

      def func_a(a, x):\n return a[1] * anp.exp(-a[0] * x)

      \n\n

      def func_b(a, x):\n return a[2] * anp.exp(-a[0] * x)

      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • priors (dict or list, optional):\npriors can either be a dictionary with integer keys and the corresponding priors as values or\na list with an entry for every parameter in the fit. The entries can either be\nObs (e.g. results from a previous fit) or strings containing a value and an error formatted like\n0.548(23), 500(40) or 0.5(0.4)
    • \n
    • silent (bool, optional):\nIf true all output to the console is omitted (default False).
    • \n
    • initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for\nnon-linear fits with many parameters. In case of correlated fits the guess is used to perform\nan uncorrelated fit which then serves as guess for the correlated fit.
    • \n
    • method (str, optional):\ncan be used to choose an alternative method for the minimization of chisquare.\nThe possible methods are the ones which can be used for scipy.optimize.minimize and\nmigrad of iminuit. If no method is specified, Levenberg-Marquard is used.\nReliable alternatives are migrad, Powell and Nelder-Mead.
    • \n
    • tol (float, optional):\ncan be used (only for combined fits and methods other than Levenberg-Marquard) to set the tolerance for convergence\nto a different value to either speed up convergence at the cost of a larger error on the fitted parameters (and possibly\ninvalid estimates for parameter uncertainties) or smaller values to get more accurate parameter values\nThe stopping criterion depends on the method, e.g. migrad: edm_max = 0.002 * tol * errordef (EDM criterion: edm < edm_max)
    • \n
    • correlated_fit (bool):\nIf True, use the full inverse covariance matrix in the definition of the chisquare cost function.\nFor details about how the covariance matrix is estimated see pyerrors.obs.covariance.\nIn practice the correlation matrix is Cholesky decomposed and inverted (instead of the covariance matrix).\nThis procedure should be numerically more stable as the correlation matrix is typically better conditioned (Jacobi preconditioning).
    • \n
    • expected_chisquare (bool):\nIf True estimates the expected chisquare which is\ncorrected by effects caused by correlated input data (default False).
    • \n
    • resplot (bool):\nIf True, a plot which displays fit, data and residuals is generated (default False).
    • \n
    • qqplot (bool):\nIf True, a quantile-quantile plot of the fit result is generated (default False).
    • \n
    • num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • output (Fit_result):\nParameters and information on the fitted result.
    • \n
    \n", "signature": "(x, y, func, priors=None, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.total_least_squares": {"fullname": "pyerrors.fits.total_least_squares", "modulename": "pyerrors.fits", "qualname": "total_least_squares", "kind": "function", "doc": "

    Performs a non-linear fit to y = func(x) and returns a list of Obs corresponding to the fit parameters.

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nlist of Obs, or a tuple of lists of Obs
    • \n
    • y (list):\nlist of Obs. The dvalues of the Obs are used as x- and yerror for the fit.
    • \n
    • func (object):\nfunc has to be of the form

      \n\n
      \n
      import autograd.numpy as anp\n\ndef func(a, x):\n   return a[0] + a[1] * x + a[2] * anp.sinh(x)\n
      \n
      \n\n

      For multiple x values func can be of the form

      \n\n
      \n
      def func(a, x):\n   (x1, x2) = x\n   return a[0] * x1 ** 2 + a[1] * x2\n
      \n
      \n\n

      It is important that all numpy functions refer to autograd.numpy, otherwise the differentiation\nwill not work.

    • \n
    • silent (bool, optional):\nIf true all output to the console is omitted (default False).
    • \n
    • initial_guess (list):\ncan provide an initial guess for the input parameters. Relevant for non-linear\nfits with many parameters.
    • \n
    • expected_chisquare (bool):\nIf true prints the expected chisquare which is\ncorrected by effects caused by correlated input data.\nThis can take a while as the full correlation matrix\nhas to be calculated (default False).
    • \n
    • num_grad (bool):\nUse numerical differentation instead of automatic differentiation to perform the error propagation (default False).
    • \n
    \n\n
    Notes
    \n\n

    Based on the orthogonal distance regression module of scipy.

    \n\n
    Returns
    \n\n
      \n
    • output (Fit_result):\nParameters and information on the fitted result.
    • \n
    \n", "signature": "(x, y, func, silent=False, **kwargs):", "funcdef": "def"}, "pyerrors.fits.fit_lin": {"fullname": "pyerrors.fits.fit_lin", "modulename": "pyerrors.fits", "qualname": "fit_lin", "kind": "function", "doc": "

    Performs a linear fit to y = n + m * x and returns two Obs n, m.

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nCan either be a list of floats in which case no xerror is assumed, or\na list of Obs, where the dvalues of the Obs are used as xerror for the fit.
    • \n
    • y (list):\nList of Obs, the dvalues of the Obs are used as yerror for the fit.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • fit_parameters (list[Obs]):\nLIist of fitted observables.
    • \n
    \n", "signature": "(x, y, **kwargs):", "funcdef": "def"}, "pyerrors.fits.qqplot": {"fullname": "pyerrors.fits.qqplot", "modulename": "pyerrors.fits", "qualname": "qqplot", "kind": "function", "doc": "

    Generates a quantile-quantile plot of the fit result which can be used to\n check if the residuals of the fit are gaussian distributed.

    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(x, o_y, func, p, title=''):", "funcdef": "def"}, "pyerrors.fits.residual_plot": {"fullname": "pyerrors.fits.residual_plot", "modulename": "pyerrors.fits", "qualname": "residual_plot", "kind": "function", "doc": "

    Generates a plot which compares the fit to the data and displays the corresponding residuals

    \n\n

    For uncorrelated data the residuals are expected to be distributed ~N(0,1).

    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(x, y, func, fit_res, title=''):", "funcdef": "def"}, "pyerrors.fits.error_band": {"fullname": "pyerrors.fits.error_band", "modulename": "pyerrors.fits", "qualname": "error_band", "kind": "function", "doc": "

    Calculate the error band for an array of sample values x, for given fit function func with optimized parameters beta.

    \n\n
    Returns
    \n\n
      \n
    • err (np.array(Obs)):\nError band for an array of sample values x
    • \n
    \n", "signature": "(x, func, beta):", "funcdef": "def"}, "pyerrors.fits.ks_test": {"fullname": "pyerrors.fits.ks_test", "modulename": "pyerrors.fits", "qualname": "ks_test", "kind": "function", "doc": "

    Performs a Kolmogorov\u2013Smirnov test for the p-values of all fit object.

    \n\n
    Parameters
    \n\n
      \n
    • objects (list):\nList of fit results to include in the analysis (optional).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(objects=None):", "funcdef": "def"}, "pyerrors.input": {"fullname": "pyerrors.input", "modulename": "pyerrors.input", "kind": "module", "doc": "

    pyerrors includes an input submodule in which input routines and parsers for the output of various numerical programs are contained.

    \n\n

    Jackknife samples

    \n\n

    For comparison with other analysis workflows pyerrors can also generate jackknife samples from an Obs object or import jackknife samples into an Obs object.\nSee pyerrors.obs.Obs.export_jackknife and pyerrors.obs.import_jackknife for details.

    \n"}, "pyerrors.input.bdio": {"fullname": "pyerrors.input.bdio", "modulename": "pyerrors.input.bdio", "kind": "module", "doc": "

    \n"}, "pyerrors.input.bdio.read_ADerrors": {"fullname": "pyerrors.input.bdio.read_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "read_ADerrors", "kind": "function", "doc": "

    Extract generic MCMC data from a bdio file

    \n\n

    read_ADerrors requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path -- path to the bdio file
    • \n
    • bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (List[Obs]):\nExtracted data
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.write_ADerrors": {"fullname": "pyerrors.input.bdio.write_ADerrors", "modulename": "pyerrors.input.bdio", "qualname": "write_ADerrors", "kind": "function", "doc": "

    Write Obs to a bdio file according to ADerrors conventions

    \n\n

    read_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path -- path to the bdio file
    • \n
    • bdio_path -- path to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • success (int):\nreturns 0 is successful
    • \n
    \n", "signature": "(obs_list, file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_mesons": {"fullname": "pyerrors.input.bdio.read_mesons", "modulename": "pyerrors.input.bdio", "qualname": "read_mesons", "kind": "function", "doc": "

    Extract mesons data from a bdio file and return it as a dictionary

    \n\n

    The dictionary can be accessed with a tuple consisting of (type, source_position, kappa1, kappa2)

    \n\n

    read_mesons requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path (str):\npath to the bdio file
    • \n
    • bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    • start (int):\nThe first configuration to be read (default 1)
    • \n
    • stop (int):\nThe last configuration to be read (default None)
    • \n
    • step (int):\nFixed step size between two measurements (default 1)
    • \n
    • alternative_ensemble_name (str):\nManually overwrite ensemble name
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (dict):\nExtracted meson data
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.bdio.read_dSdm": {"fullname": "pyerrors.input.bdio.read_dSdm", "modulename": "pyerrors.input.bdio", "qualname": "read_dSdm", "kind": "function", "doc": "

    Extract dSdm data from a bdio file and return it as a dictionary

    \n\n

    The dictionary can be accessed with a tuple consisting of (type, kappa)

    \n\n

    read_dSdm requires bdio to be compiled into a shared library. This can be achieved by\nadding the flag -fPIC to CC and changing the all target to

    \n\n

    all: bdio.o $(LIBDIR)\n gcc -shared -Wl,-soname,libbdio.so -o $(BUILDDIR)/libbdio.so $(BUILDDIR)/bdio.o\n cp $(BUILDDIR)/libbdio.so $(LIBDIR)/

    \n\n
    Parameters
    \n\n
      \n
    • file_path (str):\npath to the bdio file
    • \n
    • bdio_path (str):\npath to the shared bdio library libbdio.so (default ./libbdio.so)
    • \n
    • start (int):\nThe first configuration to be read (default 1)
    • \n
    • stop (int):\nThe last configuration to be read (default None)
    • \n
    • step (int):\nFixed step size between two measurements (default 1)
    • \n
    • alternative_ensemble_name (str):\nManually overwrite ensemble name
    • \n
    \n", "signature": "(file_path, bdio_path='./libbdio.so', **kwargs):", "funcdef": "def"}, "pyerrors.input.dobs": {"fullname": "pyerrors.input.dobs", "modulename": "pyerrors.input.dobs", "kind": "module", "doc": "

    \n"}, "pyerrors.input.dobs.create_pobs_string": {"fullname": "pyerrors.input.dobs.create_pobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_pobs_string", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to an xml string\naccording to the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • xml_str (str):\nXML formatted string of the input data
    • \n
    \n", "signature": "(obsl, name, spec='', origin='', symbol=[], enstag=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_pobs": {"fullname": "pyerrors.input.dobs.write_pobs", "modulename": "pyerrors.input.dobs", "qualname": "write_pobs", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure have to be defined on the same ensemble.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • enstag (str):\nEnstag that is written to pobs. If None, the ensemble name is used.
    • \n
    • gz (bool):\nIf True, the output is a gzipped xml. If False, the output is an xml file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(\tobsl,\tfname,\tname,\tspec='',\torigin='',\tsymbol=[],\tenstag=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_pobs": {"fullname": "pyerrors.input.dobs.read_pobs", "modulename": "pyerrors.input.dobs", "qualname": "read_pobs", "kind": "function", "doc": "

    Import a list of Obs from an xml.gz file in the Zeuthen pobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • separatior_insertion (str or int):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nNone (default): Replica names remain unchanged.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(fname, full_output=False, gz=True, separator_insertion=None):", "funcdef": "def"}, "pyerrors.input.dobs.import_dobs_string": {"fullname": "pyerrors.input.dobs.import_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "import_dobs_string", "kind": "function", "doc": "

    Import a list of Obs from a string in the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • content (str):\nXML string containing the data
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(content, full_output=False, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.read_dobs": {"fullname": "pyerrors.input.dobs.read_dobs", "modulename": "pyerrors.input.dobs", "qualname": "read_dobs", "kind": "function", "doc": "

    Import a list of Obs from an xml.gz file in the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned as list.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes XML file.
    • \n
    • separatior_insertion (str, int or bool):\nstr: replace all occurences of \"separator_insertion\" within the replica names\nby \"|%s\" % (separator_insertion) when constructing the names of the replica.\nint: Insert the separator \"|\" at the position given by separator_insertion.\nTrue (default): separator \"|\" is inserted after len(ensname), assuming that the\nensemble name is a prefix to the replica name.\nNone or False: No separator is inserted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (list[Obs]):\nImported data
    • \n
    • or
    • \n
    • res (dict):\nImported data and meta-data
    • \n
    \n", "signature": "(fname, full_output=False, gz=True, separator_insertion=True):", "funcdef": "def"}, "pyerrors.input.dobs.create_dobs_string": {"fullname": "pyerrors.input.dobs.create_dobs_string", "modulename": "pyerrors.input.dobs", "qualname": "create_dobs_string", "kind": "function", "doc": "

    Generate the string for the export of a list of Obs or structures containing Obs\nto a .xml.gz file according to the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically. The separator |is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • who (str):\nProvide the name of the person that exports the data.
    • \n
    • enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • xml_str (str):\nXML string generated from the data
    • \n
    \n", "signature": "(\tobsl,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None):", "funcdef": "def"}, "pyerrors.input.dobs.write_dobs": {"fullname": "pyerrors.input.dobs.write_dobs", "modulename": "pyerrors.input.dobs", "qualname": "write_dobs", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .xml.gz file\naccording to the Zeuthen dobs format.

    \n\n

    Tags are not written or recovered automatically. The separator | is removed from the replica names.

    \n\n
    Parameters
    \n\n
      \n
    • obsl (list):\nList of Obs that will be exported.\nThe Obs inside a structure do not have to be defined on the same set of configurations,\nbut the storage requirement is increased, if this is not the case.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • name (str):\nThe name of the observable.
    • \n
    • spec (str):\nOptional string that describes the contents of the file.
    • \n
    • origin (str):\nSpecify where the data has its origin.
    • \n
    • symbol (list):\nA list of symbols that describe the observables to be written. May be empty.
    • \n
    • who (str):\nProvide the name of the person that exports the data.
    • \n
    • enstags (dict):\nProvide alternative enstag for ensembles in the form enstags = {ename: enstag}\nOtherwise, the ensemble name is used.
    • \n
    • gz (bool):\nIf True, the output is a gzipped XML. If False, the output is a XML file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(\tobsl,\tfname,\tname,\tspec='dobs v1.0',\torigin='',\tsymbol=[],\twho=None,\tenstags=None,\tgz=True):", "funcdef": "def"}, "pyerrors.input.hadrons": {"fullname": "pyerrors.input.hadrons", "modulename": "pyerrors.input.hadrons", "kind": "module", "doc": "

    \n"}, "pyerrors.input.hadrons.read_meson_hd5": {"fullname": "pyerrors.input.hadrons.read_meson_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_meson_hd5", "kind": "function", "doc": "

    Read hadrons meson hdf5 file and extract the meson labeled 'meson'

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • meson (str):\nlabel of the meson to be extracted, standard value meson_0 which\ncorresponds to the pseudoscalar pseudoscalar two-point function.
    • \n
    • gammas (tuple of strings):\nInstrad of a meson label one can also provide a tuple of two strings\nindicating the gamma matrices at source and sink.\n(\"Gamma5\", \"Gamma5\") corresponds to the pseudoscalar pseudoscalar\ntwo-point function. The gammas argument dominateds over meson.
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • corr (Corr):\nCorrelator of the source sink combination in question.
    • \n
    \n", "signature": "(path, filestem, ens_id, meson='meson_0', idl=None, gammas=None):", "funcdef": "def"}, "pyerrors.input.hadrons.extract_t0_hd5": {"fullname": "pyerrors.input.hadrons.extract_t0_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "extract_t0_hd5", "kind": "function", "doc": "

    Read hadrons FlowObservables hdf5 file and extract t0

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • obs (str):\nlabel of the observable from which t0 should be extracted.\nOptions: 'Clover energy density' and 'Plaquette energy density'
    • \n
    • fit_range (int):\nNumber of data points left and right of the zero\ncrossing to be included in the linear fit. (Default: 5)
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    • plot_fit (bool):\nIf true, the fit for the extraction of t0 is shown together with the data.
    • \n
    \n", "signature": "(\tpath,\tfilestem,\tens_id,\tobs='Clover energy density',\tfit_range=5,\tidl=None,\t**kwargs):", "funcdef": "def"}, "pyerrors.input.hadrons.read_DistillationContraction_hd5": {"fullname": "pyerrors.input.hadrons.read_DistillationContraction_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_DistillationContraction_hd5", "kind": "function", "doc": "

    Read hadrons DistillationContraction hdf5 files in given directory structure

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the directories to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • diagrams (list):\nList of strings of the diagrams to extract, e.g. [\"direct\", \"box\", \"cross\"].
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (dict):\nextracted DistillationContration data
    • \n
    \n", "signature": "(path, ens_id, diagrams=['direct'], idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.Npr_matrix": {"fullname": "pyerrors.input.hadrons.Npr_matrix", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix", "kind": "class", "doc": "

    ndarray(shape, dtype=float, buffer=None, offset=0,\n strides=None, order=None)

    \n\n

    An array object represents a multidimensional, homogeneous array\nof fixed-size items. An associated data-type object describes the\nformat of each element in the array (its byte-order, how many bytes it\noccupies in memory, whether it is an integer, a floating point number,\nor something else, etc.)

    \n\n

    Arrays should be constructed using array, zeros or empty (refer\nto the See Also section below). The parameters given here refer to\na low-level method (ndarray(...)) for instantiating an array.

    \n\n

    For more information, refer to the numpy module and examine the\nmethods and attributes of an array.

    \n\n
    Parameters
    \n\n
      \n
    • (for the __new__ method; see Notes below)
    • \n
    • shape (tuple of ints):\nShape of created array.
    • \n
    • dtype (data-type, optional):\nAny object that can be interpreted as a numpy data type.
    • \n
    • buffer (object exposing buffer interface, optional):\nUsed to fill the array with data.
    • \n
    • offset (int, optional):\nOffset of array data in buffer.
    • \n
    • strides (tuple of ints, optional):\nStrides of data in memory.
    • \n
    • order ({'C', 'F'}, optional):\nRow-major (C-style) or column-major (Fortran-style) order.
    • \n
    \n\n
    Attributes
    \n\n
      \n
    • T (ndarray):\nTranspose of the array.
    • \n
    • data (buffer):\nThe array's elements, in memory.
    • \n
    • dtype (dtype object):\nDescribes the format of the elements in the array.
    • \n
    • flags (dict):\nDictionary containing information related to memory use, e.g.,\n'C_CONTIGUOUS', 'OWNDATA', 'WRITEABLE', etc.
    • \n
    • flat (numpy.flatiter object):\nFlattened version of the array as an iterator. The iterator\nallows assignments, e.g., x.flat = 3 (See ndarray.flat for\nassignment examples; TODO).
    • \n
    • imag (ndarray):\nImaginary part of the array.
    • \n
    • real (ndarray):\nReal part of the array.
    • \n
    • size (int):\nNumber of elements in the array.
    • \n
    • itemsize (int):\nThe memory use of each array element in bytes.
    • \n
    • nbytes (int):\nThe total number of bytes required to store the array data,\ni.e., itemsize * size.
    • \n
    • ndim (int):\nThe array's number of dimensions.
    • \n
    • shape (tuple of ints):\nShape of the array.
    • \n
    • strides (tuple of ints):\nThe step-size required to move from one element to the next in\nmemory. For example, a contiguous (3, 4) array of type\nint16 in C-order has strides (8, 2). This implies that\nto move from element to element in memory requires jumps of 2 bytes.\nTo move from row-to-row, one needs to jump 8 bytes at a time\n(2 * 4).
    • \n
    • ctypes (ctypes object):\nClass containing properties of the array needed for interaction\nwith ctypes.
    • \n
    • base (ndarray):\nIf the array is a view into another array, that array is its base\n(unless that array is also a view). The base array is where the\narray data is actually stored.
    • \n
    \n\n
    See Also
    \n\n

    array: Construct an array.
    \nzeros: Create an array, each element of which is zero.
    \nempty: Create an array, but leave its allocated memory unchanged (i.e.,\nit contains \"garbage\").
    \ndtype: Create a data-type.
    \nnumpy.typing.NDArray: An ndarray alias :term:generic <generic type>\nw.r.t. its dtype.type <numpy.dtype.type>.

    \n\n
    Notes
    \n\n

    There are two modes of creating an array using __new__:

    \n\n
      \n
    1. If buffer is None, then only shape, dtype, and order\nare used.
    2. \n
    3. If buffer is an object exposing the buffer interface, then\nall keywords are interpreted.
    4. \n
    \n\n

    No __init__ method is needed because the array is fully initialized\nafter the __new__ method.

    \n\n
    Examples
    \n\n

    These examples illustrate the low-level ndarray constructor. Refer\nto the See Also section above for easier ways of constructing an\nndarray.

    \n\n

    First mode, buffer is None:

    \n\n
    \n
    >>> np.ndarray(shape=(2,2), dtype=float, order='F')\narray([[0.0e+000, 0.0e+000], # random\n       [     nan, 2.5e-323]])\n
    \n
    \n\n

    Second mode:

    \n\n
    \n
    >>> np.ndarray((2,), buffer=np.array([1,2,3]),\n...            offset=np.int_().itemsize,\n...            dtype=int) # offset = 1*itemsize, i.e. skip first element\narray([2, 3])\n
    \n
    \n", "bases": "numpy.ndarray"}, "pyerrors.input.hadrons.Npr_matrix.g5H": {"fullname": "pyerrors.input.hadrons.Npr_matrix.g5H", "modulename": "pyerrors.input.hadrons", "qualname": "Npr_matrix.g5H", "kind": "variable", "doc": "

    Gamma_5 hermitean conjugate

    \n\n

    Uses the fact that the propagator is gamma5 hermitean, so just the\nin and out momenta of the propagator are exchanged.

    \n"}, "pyerrors.input.hadrons.read_ExternalLeg_hd5": {"fullname": "pyerrors.input.hadrons.read_ExternalLeg_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_ExternalLeg_hd5", "kind": "function", "doc": "

    Read hadrons ExternalLeg hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (Npr_matrix):\nread Cobs-matrix
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Bilinear_hd5": {"fullname": "pyerrors.input.hadrons.read_Bilinear_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Bilinear_hd5", "kind": "function", "doc": "

    Read hadrons Bilinear hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result_dict (dict[Npr_matrix]):\nextracted Bilinears
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None):", "funcdef": "def"}, "pyerrors.input.hadrons.read_Fourquark_hd5": {"fullname": "pyerrors.input.hadrons.read_Fourquark_hd5", "modulename": "pyerrors.input.hadrons", "qualname": "read_Fourquark_hd5", "kind": "function", "doc": "

    Read hadrons FourquarkFullyConnected hdf5 file and output an array of CObs

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the files to read
    • \n
    • filestem (str):\nnamestem of the files to read
    • \n
    • ens_id (str):\nname of the ensemble, required for internal bookkeeping
    • \n
    • idl (range):\nIf specified only configurations in the given range are read in.
    • \n
    • vertices (list):\nVertex functions to be extracted.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result_dict (dict):\nextracted fourquark matrizes
    • \n
    \n", "signature": "(path, filestem, ens_id, idl=None, vertices=['VA', 'AV']):", "funcdef": "def"}, "pyerrors.input.json": {"fullname": "pyerrors.input.json", "modulename": "pyerrors.input.json", "kind": "module", "doc": "

    \n"}, "pyerrors.input.json.create_json_string": {"fullname": "pyerrors.input.json.create_json_string", "modulename": "pyerrors.input.json", "qualname": "create_json_string", "kind": "function", "doc": "

    Generate the string for the export of a list of Obs or structures containing Obs\nto a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • json_string (str):\nString for export to .json(.gz) file
    • \n
    \n", "signature": "(ol, description='', indent=1):", "funcdef": "def"}, "pyerrors.input.json.dump_to_json": {"fullname": "pyerrors.input.json.dump_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_to_json", "kind": "function", "doc": "

    Export a list of Obs or structures containing Obs to a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • ol (list):\nList of objects that will be exported. At the moment, these objects can be\neither of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    • gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • Null
    • \n
    \n", "signature": "(ol, fname, description='', indent=1, gz=True):", "funcdef": "def"}, "pyerrors.input.json.import_json_string": {"fullname": "pyerrors.input.json.import_json_string", "modulename": "pyerrors.input.json", "qualname": "import_json_string", "kind": "function", "doc": "

    Reconstruct a list of Obs or structures containing Obs from a json string.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.

    \n\n
    Parameters
    \n\n
      \n
    • json_string (str):\njson string containing the data.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nreconstructed list of observables from the json string
    • \n
    • or
    • \n
    • result (Obs):\nonly one observable if the list only has one entry
    • \n
    • or
    • \n
    • result (dict):\nif full_output=True
    • \n
    \n", "signature": "(json_string, verbose=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.load_json": {"fullname": "pyerrors.input.json.load_json", "modulename": "pyerrors.input.json", "qualname": "load_json", "kind": "function", "doc": "

    Import a list of Obs or structures containing Obs from a .json(.gz) file.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr\nIf the list contains only one element, it is unpacked from the list.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nreconstructed list of observables from the json string
    • \n
    • or
    • \n
    • result (Obs):\nonly one observable if the list only has one entry
    • \n
    • or
    • \n
    • result (dict):\nif full_output=True
    • \n
    \n", "signature": "(fname, verbose=True, gz=True, full_output=False):", "funcdef": "def"}, "pyerrors.input.json.dump_dict_to_json": {"fullname": "pyerrors.input.json.dump_dict_to_json", "modulename": "pyerrors.input.json", "qualname": "dump_dict_to_json", "kind": "function", "doc": "

    Export a dict of Obs or structures containing Obs to a .json(.gz) file

    \n\n
    Parameters
    \n\n
      \n
    • od (dict):\nDict of JSON valid structures and objects that will be exported.\nAt the moment, these objects can be either of: Obs, list, numpy.ndarray, Corr.\nAll Obs inside a structure have to be defined on the same set of configurations.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • description (str):\nOptional string that describes the contents of the json file.
    • \n
    • indent (int):\nSpecify the indentation level of the json file. None or 0 is permissible and\nsaves disk space.
    • \n
    • reps (str):\nSpecify the structure of the placeholder in exported dict to be reps[0-9]+.
    • \n
    • gz (bool):\nIf True, the output is a gzipped json. If False, the output is a json file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(od, fname, description='', indent=1, reps='DICTOBS', gz=True):", "funcdef": "def"}, "pyerrors.input.json.load_json_dict": {"fullname": "pyerrors.input.json.load_json_dict", "modulename": "pyerrors.input.json", "qualname": "load_json_dict", "kind": "function", "doc": "

    Import a dict of Obs or structures containing Obs from a .json(.gz) file.

    \n\n

    The following structures are supported: Obs, list, numpy.ndarray, Corr

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • verbose (bool):\nPrint additional information that was written to the file.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    • full_output (bool):\nIf True, a dict containing auxiliary information and the data is returned.\nIf False, only the data is returned.
    • \n
    • reps (str):\nSpecify the structure of the placeholder in imported dict to be reps[0-9]+.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (Obs / list / Corr):\nRead data
    • \n
    • or
    • \n
    • data (dict):\nRead data and meta-data
    • \n
    \n", "signature": "(fname, verbose=True, gz=True, full_output=False, reps='DICTOBS'):", "funcdef": "def"}, "pyerrors.input.misc": {"fullname": "pyerrors.input.misc", "modulename": "pyerrors.input.misc", "kind": "module", "doc": "

    \n"}, "pyerrors.input.misc.fit_t0": {"fullname": "pyerrors.input.misc.fit_t0", "modulename": "pyerrors.input.misc", "qualname": "fit_t0", "kind": "function", "doc": "

    \n", "signature": "(t2E_dict, fit_range, plot_fit=False):", "funcdef": "def"}, "pyerrors.input.misc.read_pbp": {"fullname": "pyerrors.input.misc.read_pbp", "modulename": "pyerrors.input.misc", "qualname": "read_pbp", "kind": "function", "doc": "

    Read pbp format from given folder structure.

    \n\n
    Parameters
    \n\n
      \n
    • r_start (list):\nlist which contains the first config to be read for each replicum
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nlist of observables read
    • \n
    \n", "signature": "(path, prefix, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD": {"fullname": "pyerrors.input.openQCD", "modulename": "pyerrors.input.openQCD", "kind": "module", "doc": "

    \n"}, "pyerrors.input.openQCD.read_rwms": {"fullname": "pyerrors.input.openQCD.read_rwms", "modulename": "pyerrors.input.openQCD", "qualname": "read_rwms", "kind": "function", "doc": "

    Read rwms format from given folder structure. Returns a list of length nrw

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath that contains the data files
    • \n
    • prefix (str):\nall files in path that start with prefix are considered as input files.\nMay be used together postfix to consider only special file endings.\nPrefix is ignored, if the keyword 'files' is used.
    • \n
    • version (str):\nversion of openQCD, default 2.0
    • \n
    • names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum
    • \n
    • r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.ms1' for openQCD-files
    • \n
    • files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
    • \n
    • print_err (bool):\nPrint additional information that is useful for debugging.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • rwms (Obs):\nReweighting factors read
    • \n
    \n", "signature": "(path, prefix, version='2.0', names=None, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.extract_t0": {"fullname": "pyerrors.input.openQCD.extract_t0", "modulename": "pyerrors.input.openQCD", "qualname": "extract_t0", "kind": "function", "doc": "

    Extract t0 from given .ms.dat files. Returns t0 as Obs.

    \n\n

    It is assumed that all boundary effects have\nsufficiently decayed at x0=xmin.\nThe data around the zero crossing of t^2 - 0.3\nis fitted with a linear function\nfrom which the exact root is extracted.

    \n\n

    It is assumed that one measurement is performed for each config.\nIf this is not the case, the resulting idl, as well as the handling\nof r_start, r_stop and r_step is wrong and the user has to correct\nthis in the resulting observable.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nPath to .ms.dat files
    • \n
    • prefix (str):\nEnsemble prefix
    • \n
    • dtr_read (int):\nDetermines how many trajectories should be skipped\nwhen reading the ms.dat files.\nCorresponds to dtr_cnfg / dtr_ms in the openQCD input file.
    • \n
    • xmin (int):\nFirst timeslice where the boundary\neffects have sufficiently decayed.
    • \n
    • spatial_extent (int):\nspatial extent of the lattice, required for normalization.
    • \n
    • fit_range (int):\nNumber of data points left and right of the zero\ncrossing to be included in the linear fit. (Default: 5)
    • \n
    • postfix (str):\nPostfix of measurement file (Default: ms)
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • r_step (int):\ninteger that defines a fixed step size between two measurements (in units of configs)\nIf not given, r_step=1 is assumed.
    • \n
    • plaquette (bool):\nIf true extract the plaquette estimate of t0 instead.
    • \n
    • names (list):\nlist of names that is assigned to the data according according\nto the order in the file list. Use careful, if you do not provide file names!
    • \n
    • files (list):\nlist which contains the filenames to be read. No automatic detection of\nfiles performed if given.
    • \n
    • plot_fit (bool):\nIf true, the fit for the extraction of t0 is shown together with the data.
    • \n
    • assume_thermalization (bool):\nIf True: If the first record divided by the distance between two measurements is larger than\n1, it is assumed that this is due to thermalization and the first measurement belongs\nto the first config (default).\nIf False: The config numbers are assumed to be traj_number // difference
    • \n
    \n\n
    Returns
    \n\n
      \n
    • t0 (Obs):\nExtracted t0
    • \n
    \n", "signature": "(\tpath,\tprefix,\tdtr_read,\txmin,\tspatial_extent,\tfit_range=5,\tpostfix='ms',\t**kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop": {"fullname": "pyerrors.input.openQCD.read_qtop", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop", "kind": "function", "doc": "

    Read the topologial charge based on openQCD gradient flow measurements.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files.
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • version (str):\nEither openQCD or sfqcd, depending on the data.
    • \n
    • L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
    • \n
    • integer_charge (bool):\nIf True, the charge is rounded towards the nearest integer on each config.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (Obs):\nRead topological charge
    • \n
    \n", "signature": "(path, prefix, c, dtr_cnfg=1, version='openQCD', **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_gf_coupling": {"fullname": "pyerrors.input.openQCD.read_gf_coupling", "modulename": "pyerrors.input.openQCD", "qualname": "read_gf_coupling", "kind": "function", "doc": "

    Read the gradient flow coupling based on sfqcd gradient flow measurements. See 1607.06423 for details.

    \n\n

    Note: The current implementation only works for c=0.3 and T=L. The definition of the coupling in 1607.06423 requires projection to topological charge zero which is not done within this function but has to be performed in a separate step.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat.\nIgnored if file names are passed explicitly via keyword files.
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L.
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of measurements\nbetween two configs.\nIf it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • r_start (list):\nlist which contains the first config to be read for each replicum.
    • \n
    • r_stop (list):\nlist which contains the last config to be read for each replicum.
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length.
    • \n
    • postfix (str):\npostfix of the file to read, e.g. '.gfms.dat' for openQCD-files
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for the coupling. If False, the Wilson flow is used.
    • \n
    \n", "signature": "(path, prefix, c, dtr_cnfg=1, Zeuthen_flow=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.qtop_projection": {"fullname": "pyerrors.input.openQCD.qtop_projection", "modulename": "pyerrors.input.openQCD", "qualname": "qtop_projection", "kind": "function", "doc": "

    Returns the projection to the topological charge sector defined by target.

    \n\n
    Parameters
    \n\n
      \n
    • path (Obs):\nTopological charge.
    • \n
    • target (int):\nSpecifies the topological sector to be reweighted to (default 0)
    • \n
    \n\n
    Returns
    \n\n
      \n
    • reto (Obs):\nprojection to the topological charge sector defined by target
    • \n
    \n", "signature": "(qtop, target=0):", "funcdef": "def"}, "pyerrors.input.openQCD.read_qtop_sector": {"fullname": "pyerrors.input.openQCD.read_qtop_sector", "modulename": "pyerrors.input.openQCD", "qualname": "read_qtop_sector", "kind": "function", "doc": "

    Constructs reweighting factors to a specified topological sector.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath of the measurement files
    • \n
    • prefix (str):\nprefix of the measurement files, e.g. _id0_r0.ms.dat
    • \n
    • c (double):\nSmearing radius in units of the lattice extent, c = sqrt(8 t0) / L
    • \n
    • target (int):\nSpecifies the topological sector to be reweighted to (default 0)
    • \n
    • dtr_cnfg (int):\n(optional) parameter that specifies the number of trajectories\nbetween two configs.\nif it is not set, the distance between two measurements\nin the file is assumed to be the distance between two configurations.
    • \n
    • steps (int):\n(optional) Distance between two configurations in units of trajectories /\n cycles. Assumed to be the distance between two measurements * dtr_cnfg if not given
    • \n
    • version (str):\nversion string of the openQCD (sfqcd) version used to create\nthe ensemble. Default is 2.0. May also be set to sfqcd.
    • \n
    • L (int):\nspatial length of the lattice in L/a.\nHAS to be set if version != sfqcd, since openQCD does not provide\nthis in the header
    • \n
    • r_start (list):\noffset of the first ensemble, making it easier to match\nlater on with other Obs
    • \n
    • r_stop (list):\nlast configurations that need to be read (per replicum)
    • \n
    • files (list):\nspecify the exact files that need to be read\nfrom path, practical if e.g. only one replicum is needed
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
    • \n
    • Zeuthen_flow (bool):\n(optional) If True, the Zeuthen flow is used for Qtop. Only possible\nfor version=='sfqcd' If False, the Wilson flow is used.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • reto (Obs):\nprojection to the topological charge sector defined by target
    • \n
    \n", "signature": "(path, prefix, c, target=0, **kwargs):", "funcdef": "def"}, "pyerrors.input.openQCD.read_ms5_xsf": {"fullname": "pyerrors.input.openQCD.read_ms5_xsf", "modulename": "pyerrors.input.openQCD", "qualname": "read_ms5_xsf", "kind": "function", "doc": "

    Read data from files in the specified directory with the specified prefix and quark combination extension, and return a Corr object containing the data.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nThe directory to search for the files in.
    • \n
    • prefix (str):\nThe prefix to match the files against.
    • \n
    • qc (str):\nThe quark combination extension to match the files against.
    • \n
    • corr (str):\nThe correlator to extract data for.
    • \n
    • sep (str, optional):\nThe separator to use when parsing the replika names.
    • \n
    • **kwargs: Additional keyword arguments. The following keyword arguments are recognized:

      \n\n
        \n
      • names (List[str]): A list of names to use for the replicas.
      • \n
    • \n
    \n\n
    Returns
    \n\n
      \n
    • Corr: A complex valued Corr object containing the data read from the files. In case of boudary to bulk correlators.
    • \n
    • or
    • \n
    • CObs: A complex valued CObs object containing the data read from the files. In case of boudary to boundary correlators.
    • \n
    \n\n
    Raises
    \n\n
      \n
    • FileNotFoundError: If no files matching the specified prefix and quark combination extension are found in the specified directory.
    • \n
    • IOError: If there is an error reading a file.
    • \n
    • struct.error: If there is an error unpacking binary data.
    • \n
    \n", "signature": "(path, prefix, qc, corr, sep='r', **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas": {"fullname": "pyerrors.input.pandas", "modulename": "pyerrors.input.pandas", "kind": "module", "doc": "

    \n"}, "pyerrors.input.pandas.to_sql": {"fullname": "pyerrors.input.pandas.to_sql", "modulename": "pyerrors.input.pandas", "qualname": "to_sql", "kind": "function", "doc": "

    Write DataFrame including Obs or Corr valued columns to sqlite database.

    \n\n
    Parameters
    \n\n
      \n
    • df (pandas.DataFrame):\nDataframe to be written to the database.
    • \n
    • table_name (str):\nName of the table in the database.
    • \n
    • db (str):\nPath to the sqlite database.
    • \n
    • if exists (str):\nHow to behave if table already exists. Options 'fail', 'replace', 'append'.
    • \n
    • gz (bool):\nIf True the json strings are gzipped.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(df, table_name, db, if_exists='fail', gz=True, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.read_sql": {"fullname": "pyerrors.input.pandas.read_sql", "modulename": "pyerrors.input.pandas", "qualname": "read_sql", "kind": "function", "doc": "

    Execute SQL query on sqlite database and obtain DataFrame including Obs or Corr valued columns.

    \n\n
    Parameters
    \n\n
      \n
    • sql (str):\nSQL query to be executed.
    • \n
    • db (str):\nPath to the sqlite database.
    • \n
    • auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (pandas.DataFrame):\nDataframe with the content of the sqlite database.
    • \n
    \n", "signature": "(sql, db, auto_gamma=False, **kwargs):", "funcdef": "def"}, "pyerrors.input.pandas.dump_df": {"fullname": "pyerrors.input.pandas.dump_df", "modulename": "pyerrors.input.pandas", "qualname": "dump_df", "kind": "function", "doc": "

    Exports a pandas DataFrame containing Obs valued columns to a (gzipped) csv file.

    \n\n

    Before making use of pandas to_csv functionality Obs objects are serialized via the standardized\njson format of pyerrors.

    \n\n
    Parameters
    \n\n
      \n
    • df (pandas.DataFrame):\nDataframe to be dumped to a file.
    • \n
    • fname (str):\nFilename of the output file.
    • \n
    • gz (bool):\nIf True, the output is a gzipped csv file. If False, the output is a csv file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(df, fname, gz=True):", "funcdef": "def"}, "pyerrors.input.pandas.load_df": {"fullname": "pyerrors.input.pandas.load_df", "modulename": "pyerrors.input.pandas", "qualname": "load_df", "kind": "function", "doc": "

    Imports a pandas DataFrame from a csv.(gz) file in which Obs objects are serialized as json strings.

    \n\n
    Parameters
    \n\n
      \n
    • fname (str):\nFilename of the input file.
    • \n
    • auto_gamma (bool):\nIf True applies the gamma_method to all imported Obs objects with the default parameters for\nthe error analysis. Default False.
    • \n
    • gz (bool):\nIf True, assumes that data is gzipped. If False, assumes JSON file.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • data (pandas.DataFrame):\nDataframe with the content of the sqlite database.
    • \n
    \n", "signature": "(fname, auto_gamma=False, gz=True):", "funcdef": "def"}, "pyerrors.input.sfcf": {"fullname": "pyerrors.input.sfcf", "modulename": "pyerrors.input.sfcf", "kind": "module", "doc": "

    \n"}, "pyerrors.input.sfcf.read_sfcf": {"fullname": "pyerrors.input.sfcf.read_sfcf", "modulename": "pyerrors.input.sfcf", "qualname": "read_sfcf", "kind": "function", "doc": "

    Read sfcf files from given folder structure.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\nPath to the sfcf files.
    • \n
    • prefix (str):\nPrefix of the sfcf files.
    • \n
    • name (str):\nName of the correlation function to read.
    • \n
    • quarks (str):\nLabel of the quarks used in the sfcf input file. e.g. \"quark quark\"\nfor version 0.0 this does NOT need to be given with the typical \" - \"\nthat is present in the output file,\nthis is done automatically for this version
    • \n
    • corr_type (str):\nType of correlation function to read. Can be\n
        \n
      • 'bi' for boundary-inner
      • \n
      • 'bb' for boundary-boundary
      • \n
      • 'bib' for boundary-inner-boundary
      • \n
    • \n
    • noffset (int):\nOffset of the source (only relevant when wavefunctions are used)
    • \n
    • wf (int):\nID of wave function
    • \n
    • wf2 (int):\nID of the second wavefunction\n(only relevant for boundary-to-boundary correlation functions)
    • \n
    • im (bool):\nif True, read imaginary instead of real part\nof the correlation function.
    • \n
    • names (list):\nAlternative labeling for replicas/ensembles.\nHas to have the appropriate length
    • \n
    • ens_name (str):\nreplaces the name of the ensemble
    • \n
    • version (str):\nversion of SFCF, with which the measurement was done.\nif the compact output option (-c) was specified,\nappend a \"c\" to the version (e.g. \"1.0c\")\nif the append output option (-a) was specified,\nappend an \"a\" to the version
    • \n
    • cfg_separator (str):\nString that separates the ensemble identifier from the configuration number (default 'n').
    • \n
    • replica (list):\nlist of replica to be read, default is all
    • \n
    • files (list):\nlist of files to be read per replica, default is all.\nfor non-compact output format, hand the folders to be read here.
    • \n
    • check_configs (list[list[int]]):\nlist of list of supposed configs, eg. [range(1,1000)]\nfor one replicum with 1000 configs
    • \n
    \n\n
    Returns
    \n\n
      \n
    • result (list[Obs]):\nlist of Observables with length T, observable per timeslice.\nbb-type correlators have length 1.
    • \n
    \n", "signature": "(\tpath,\tprefix,\tname,\tquarks='.*',\tcorr_type='bi',\tnoffset=0,\twf=0,\twf2=0,\tversion='1.0c',\tcfg_separator='n',\tsilent=False,\t**kwargs):", "funcdef": "def"}, "pyerrors.input.utils": {"fullname": "pyerrors.input.utils", "modulename": "pyerrors.input.utils", "kind": "module", "doc": "

    \n"}, "pyerrors.input.utils.sort_names": {"fullname": "pyerrors.input.utils.sort_names", "modulename": "pyerrors.input.utils", "qualname": "sort_names", "kind": "function", "doc": "

    Sorts a list of names of replika with searches for r and id in the replikum string.\nIf this search fails, a fallback method is used,\nwhere the strings are simply compared and the first diffeing numeral is used for differentiation.

    \n\n
    Parameters
    \n\n
      \n
    • ll (list):\nlist to sort
    • \n
    \n\n
    Returns
    \n\n
      \n
    • ll (list):\nsorted list
    • \n
    \n", "signature": "(ll):", "funcdef": "def"}, "pyerrors.input.utils.check_idl": {"fullname": "pyerrors.input.utils.check_idl", "modulename": "pyerrors.input.utils", "qualname": "check_idl", "kind": "function", "doc": "

    Checks if list of configurations is contained in an idl

    \n\n
    Parameters
    \n\n
      \n
    • idl (range or list):\nidl of the current replicum
    • \n
    • che (list):\nlist of configurations to be checked against
    • \n
    \n\n
    Returns
    \n\n
      \n
    • miss_str (str):\nstring with integers of which idls are missing
    • \n
    \n", "signature": "(idl, che):", "funcdef": "def"}, "pyerrors.linalg": {"fullname": "pyerrors.linalg", "modulename": "pyerrors.linalg", "kind": "module", "doc": "

    \n"}, "pyerrors.linalg.matmul": {"fullname": "pyerrors.linalg.matmul", "modulename": "pyerrors.linalg", "qualname": "matmul", "kind": "function", "doc": "

    Matrix multiply all operands.

    \n\n
    Parameters
    \n\n
      \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    • This implementation is faster compared to standard multiplication via the @ operator.
    • \n
    \n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.jack_matmul": {"fullname": "pyerrors.linalg.jack_matmul", "modulename": "pyerrors.linalg", "qualname": "jack_matmul", "kind": "function", "doc": "

    Matrix multiply both operands making use of the jackknife approximation.

    \n\n
    Parameters
    \n\n
      \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    • For large matrices this is considerably faster compared to matmul.
    • \n
    \n", "signature": "(*operands):", "funcdef": "def"}, "pyerrors.linalg.einsum": {"fullname": "pyerrors.linalg.einsum", "modulename": "pyerrors.linalg", "qualname": "einsum", "kind": "function", "doc": "

    Wrapper for numpy.einsum

    \n\n
    Parameters
    \n\n
      \n
    • subscripts (str):\nSubscripts for summation (see numpy documentation for details)
    • \n
    • operands (numpy.ndarray):\nArbitrary number of 2d-numpy arrays which can be real or complex\nObs valued.
    • \n
    \n", "signature": "(subscripts, *operands):", "funcdef": "def"}, "pyerrors.linalg.inv": {"fullname": "pyerrors.linalg.inv", "modulename": "pyerrors.linalg", "qualname": "inv", "kind": "function", "doc": "

    Inverse of Obs or CObs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.cholesky": {"fullname": "pyerrors.linalg.cholesky", "modulename": "pyerrors.linalg", "qualname": "cholesky", "kind": "function", "doc": "

    Cholesky decomposition of Obs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.det": {"fullname": "pyerrors.linalg.det", "modulename": "pyerrors.linalg", "qualname": "det", "kind": "function", "doc": "

    Determinant of Obs valued matrices.

    \n", "signature": "(x):", "funcdef": "def"}, "pyerrors.linalg.eigh": {"fullname": "pyerrors.linalg.eigh", "modulename": "pyerrors.linalg", "qualname": "eigh", "kind": "function", "doc": "

    Computes the eigenvalues and eigenvectors of a given hermitian matrix of Obs according to np.linalg.eigh.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.eig": {"fullname": "pyerrors.linalg.eig", "modulename": "pyerrors.linalg", "qualname": "eig", "kind": "function", "doc": "

    Computes the eigenvalues of a given matrix of Obs according to np.linalg.eig.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.pinv": {"fullname": "pyerrors.linalg.pinv", "modulename": "pyerrors.linalg", "qualname": "pinv", "kind": "function", "doc": "

    Computes the Moore-Penrose pseudoinverse of a matrix of Obs.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.linalg.svd": {"fullname": "pyerrors.linalg.svd", "modulename": "pyerrors.linalg", "qualname": "svd", "kind": "function", "doc": "

    Computes the singular value decomposition of a matrix of Obs.

    \n", "signature": "(obs, **kwargs):", "funcdef": "def"}, "pyerrors.misc": {"fullname": "pyerrors.misc", "modulename": "pyerrors.misc", "kind": "module", "doc": "

    \n"}, "pyerrors.misc.print_config": {"fullname": "pyerrors.misc.print_config", "modulename": "pyerrors.misc", "qualname": "print_config", "kind": "function", "doc": "

    Print information about version of python, pyerrors and dependencies.

    \n", "signature": "():", "funcdef": "def"}, "pyerrors.misc.errorbar": {"fullname": "pyerrors.misc.errorbar", "modulename": "pyerrors.misc", "qualname": "errorbar", "kind": "function", "doc": "

    pyerrors wrapper for the errorbars method of matplotlib

    \n\n
    Parameters
    \n\n
      \n
    • x (list):\nA list of x-values which can be Obs.
    • \n
    • y (list):\nA list of y-values which can be Obs.
    • \n
    • axes ((matplotlib.pyplot.axes)):\nThe axes to plot on. default is plt.
    • \n
    \n", "signature": "(\tx,\ty,\taxes=<module 'matplotlib.pyplot' from '/opt/hostedtoolcache/Python/3.10.11/x64/lib/python3.10/site-packages/matplotlib/pyplot.py'>,\t**kwargs):", "funcdef": "def"}, "pyerrors.misc.dump_object": {"fullname": "pyerrors.misc.dump_object", "modulename": "pyerrors.misc", "qualname": "dump_object", "kind": "function", "doc": "

    Dump object into pickle file.

    \n\n
    Parameters
    \n\n
      \n
    • obj (object):\nobject to be saved in the pickle file
    • \n
    • name (str):\nname of the file
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n\n
    Returns
    \n\n
      \n
    • None
    • \n
    \n", "signature": "(obj, name, **kwargs):", "funcdef": "def"}, "pyerrors.misc.load_object": {"fullname": "pyerrors.misc.load_object", "modulename": "pyerrors.misc", "qualname": "load_object", "kind": "function", "doc": "

    Load object from pickle file.

    \n\n
    Parameters
    \n\n
      \n
    • path (str):\npath to the file
    • \n
    \n\n
    Returns
    \n\n
      \n
    • object (Obs):\nLoaded Object
    • \n
    \n", "signature": "(path):", "funcdef": "def"}, "pyerrors.misc.pseudo_Obs": {"fullname": "pyerrors.misc.pseudo_Obs", "modulename": "pyerrors.misc", "qualname": "pseudo_Obs", "kind": "function", "doc": "

    Generate an Obs object with given value, dvalue and name for test purposes

    \n\n
    Parameters
    \n\n
      \n
    • value (float):\ncentral value of the Obs to be generated.
    • \n
    • dvalue (float):\nerror of the Obs to be generated.
    • \n
    • name (str):\nname of the ensemble for which the Obs is to be generated.
    • \n
    • samples (int):\nnumber of samples for the Obs (default 1000).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (Obs):\nGenerated Observable
    • \n
    \n", "signature": "(value, dvalue, name, samples=1000):", "funcdef": "def"}, "pyerrors.misc.gen_correlated_data": {"fullname": "pyerrors.misc.gen_correlated_data", "modulename": "pyerrors.misc", "qualname": "gen_correlated_data", "kind": "function", "doc": "

    Generate observables with given covariance and autocorrelation times.

    \n\n
    Parameters
    \n\n
      \n
    • means (list):\nlist containing the mean value of each observable.
    • \n
    • cov (numpy.ndarray):\ncovariance matrix for the data to be generated.
    • \n
    • name (str):\nensemble name for the data to be geneated.
    • \n
    • tau (float or list):\ncan either be a real number or a list with an entry for\nevery dataset.
    • \n
    • samples (int):\nnumber of samples to be generated for each observable.
    • \n
    \n\n
    Returns
    \n\n
      \n
    • corr_obs (list[Obs]):\nGenerated observable list
    • \n
    \n", "signature": "(means, cov, name, tau=0.5, samples=1000):", "funcdef": "def"}, "pyerrors.mpm": {"fullname": "pyerrors.mpm", "modulename": "pyerrors.mpm", "kind": "module", "doc": "

    \n"}, "pyerrors.mpm.matrix_pencil_method": {"fullname": "pyerrors.mpm.matrix_pencil_method", "modulename": "pyerrors.mpm", "qualname": "matrix_pencil_method", "kind": "function", "doc": "

    Matrix pencil method to extract k energy levels from data

    \n\n

    Implementation of the matrix pencil method based on\neq. (2.17) of Y. Hua, T. K. Sarkar, IEEE Trans. Acoust. 38, 814-824 (1990)

    \n\n
    Parameters
    \n\n
      \n
    • data (list):\ncan be a list of Obs for the analysis of a single correlator, or a list of lists\nof Obs if several correlators are to analyzed at once.
    • \n
    • k (int):\nNumber of states to extract (default 1).
    • \n
    • p (int):\nmatrix pencil parameter which filters noise. The optimal value is expected between\nlen(data)/3 and 2*len(data)/3. The computation is more expensive the closer p is\nto len(data)/2 but could possibly suppress more noise (default len(data)//2).
    • \n
    \n\n
    Returns
    \n\n
      \n
    • energy_levels (list[Obs]):\nExtracted energy levels
    • \n
    \n", "signature": "(corrs, k=1, p=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs": {"fullname": "pyerrors.obs", "modulename": "pyerrors.obs", "kind": "module", "doc": "

    \n"}, "pyerrors.obs.Obs": {"fullname": "pyerrors.obs.Obs", "modulename": "pyerrors.obs", "qualname": "Obs", "kind": "class", "doc": "

    Class for a general observable.

    \n\n

    Instances of Obs are the basic objects of a pyerrors error analysis.\nThey are initialized with a list which contains arrays of samples for\ndifferent ensembles/replica and another list of same length which contains\nthe names of the ensembles/replica. Mathematical operations can be\nperformed on instances. The result is another instance of Obs. The error of\nan instance can be computed with the gamma_method. Also contains additional\nmethods for output and visualization of the error calculation.

    \n\n
    Attributes
    \n\n
      \n
    • S_global (float):\nStandard value for S (default 2.0)
    • \n
    • S_dict (dict):\nDictionary for S values. If an entry for a given ensemble\nexists this overwrites the standard value for that ensemble.
    • \n
    • tau_exp_global (float):\nStandard value for tau_exp (default 0.0)
    • \n
    • tau_exp_dict (dict):\nDictionary for tau_exp values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
    • \n
    • N_sigma_global (float):\nStandard value for N_sigma (default 1.0)
    • \n
    • N_sigma_dict (dict):\nDictionary for N_sigma values. If an entry for a given ensemble exists\nthis overwrites the standard value for that ensemble.
    • \n
    \n"}, "pyerrors.obs.Obs.__init__": {"fullname": "pyerrors.obs.Obs.__init__", "modulename": "pyerrors.obs", "qualname": "Obs.__init__", "kind": "function", "doc": "

    Initialize Obs object.

    \n\n
    Parameters
    \n\n
      \n
    • samples (list):\nlist of numpy arrays containing the Monte Carlo samples
    • \n
    • names (list):\nlist of strings labeling the individual samples
    • \n
    • idl (list, optional):\nlist of ranges or lists on which the samples are defined
    • \n
    \n", "signature": "(samples, names, idl=None, **kwargs)"}, "pyerrors.obs.Obs.gamma_method": {"fullname": "pyerrors.obs.Obs.gamma_method", "modulename": "pyerrors.obs", "qualname": "Obs.gamma_method", "kind": "function", "doc": "

    Estimate the error and related properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
    • \n
    • tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
    • \n
    • N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
    • \n
    • fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
    • \n
    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.gm": {"fullname": "pyerrors.obs.Obs.gm", "modulename": "pyerrors.obs", "qualname": "Obs.gm", "kind": "function", "doc": "

    Estimate the error and related properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • S (float):\nspecifies a custom value for the parameter S (default 2.0).\nIf set to 0 it is assumed that the data exhibits no\nautocorrelation. In this case the error estimates coincides\nwith the sample standard error.
    • \n
    • tau_exp (float):\npositive value triggers the critical slowing down analysis\n(default 0.0).
    • \n
    • N_sigma (float):\nnumber of standard deviations from zero until the tail is\nattached to the autocorrelation function (default 1).
    • \n
    • fft (bool):\ndetermines whether the fft algorithm is used for the computation\nof the autocorrelation function (default True)
    • \n
    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.details": {"fullname": "pyerrors.obs.Obs.details", "modulename": "pyerrors.obs", "qualname": "Obs.details", "kind": "function", "doc": "

    Output detailed properties of the Obs.

    \n\n
    Parameters
    \n\n
      \n
    • ens_content (bool):\nprint details about the ensembles and replica if true.
    • \n
    \n", "signature": "(self, ens_content=True):", "funcdef": "def"}, "pyerrors.obs.Obs.reweight": {"fullname": "pyerrors.obs.Obs.reweight", "modulename": "pyerrors.obs", "qualname": "Obs.reweight", "kind": "function", "doc": "

    Reweight the obs with given rewighting factors.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
    • \n
    \n", "signature": "(self, weight):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero_within_error": {"fullname": "pyerrors.obs.Obs.is_zero_within_error", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero_within_error", "kind": "function", "doc": "

    Checks whether the observable is zero within 'sigma' standard errors.

    \n\n
    Parameters
    \n\n
      \n
    • sigma (int):\nNumber of standard errors used for the check.
    • \n
    • Works only properly when the gamma method was run.
    • \n
    \n", "signature": "(self, sigma=1):", "funcdef": "def"}, "pyerrors.obs.Obs.is_zero": {"fullname": "pyerrors.obs.Obs.is_zero", "modulename": "pyerrors.obs", "qualname": "Obs.is_zero", "kind": "function", "doc": "

    Checks whether the observable is zero within a given tolerance.

    \n\n
    Parameters
    \n\n
      \n
    • atol (float):\nAbsolute tolerance (for details see numpy documentation).
    • \n
    \n", "signature": "(self, atol=1e-10):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_tauint": {"fullname": "pyerrors.obs.Obs.plot_tauint", "modulename": "pyerrors.obs", "qualname": "Obs.plot_tauint", "kind": "function", "doc": "

    Plot integrated autocorrelation time for each ensemble.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rho": {"fullname": "pyerrors.obs.Obs.plot_rho", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rho", "kind": "function", "doc": "

    Plot normalized autocorrelation function time for each ensemble.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_rep_dist": {"fullname": "pyerrors.obs.Obs.plot_rep_dist", "modulename": "pyerrors.obs", "qualname": "Obs.plot_rep_dist", "kind": "function", "doc": "

    Plot replica distribution for each ensemble with more than one replicum.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_history": {"fullname": "pyerrors.obs.Obs.plot_history", "modulename": "pyerrors.obs", "qualname": "Obs.plot_history", "kind": "function", "doc": "

    Plot derived Monte Carlo history for each ensemble

    \n\n
    Parameters
    \n\n
      \n
    • expand (bool):\nshow expanded history for irregular Monte Carlo chains (default: True).
    • \n
    \n", "signature": "(self, expand=True):", "funcdef": "def"}, "pyerrors.obs.Obs.plot_piechart": {"fullname": "pyerrors.obs.Obs.plot_piechart", "modulename": "pyerrors.obs", "qualname": "Obs.plot_piechart", "kind": "function", "doc": "

    Plot piechart which shows the fractional contribution of each\nensemble to the error and returns a dictionary containing the fractions.

    \n\n
    Parameters
    \n\n
      \n
    • save (str):\nsaves the figure to a file named 'save' if.
    • \n
    \n", "signature": "(self, save=None):", "funcdef": "def"}, "pyerrors.obs.Obs.dump": {"fullname": "pyerrors.obs.Obs.dump", "modulename": "pyerrors.obs", "qualname": "Obs.dump", "kind": "function", "doc": "

    Dump the Obs to a file 'name' of chosen format.

    \n\n
    Parameters
    \n\n
      \n
    • filename (str):\nname of the file to be saved.
    • \n
    • datatype (str):\nFormat of the exported file. Supported formats include\n\"json.gz\" and \"pickle\"
    • \n
    • description (str):\nDescription for output file, only relevant for json.gz format.
    • \n
    • path (str):\nspecifies a custom path for the file (default '.')
    • \n
    \n", "signature": "(self, filename, datatype='json.gz', description='', **kwargs):", "funcdef": "def"}, "pyerrors.obs.Obs.export_jackknife": {"fullname": "pyerrors.obs.Obs.export_jackknife", "modulename": "pyerrors.obs", "qualname": "Obs.export_jackknife", "kind": "function", "doc": "

    Export jackknife samples from the Obs

    \n\n
    Returns
    \n\n
      \n
    • numpy.ndarray: Returns a numpy array of length N + 1 where N is the number of samples\nfor the given ensemble and replicum. The zeroth entry of the array contains\nthe mean value of the Obs, entries 1 to N contain the N jackknife samples\nderived from the Obs. The current implementation only works for observables\ndefined on exactly one ensemble and replicum. The derived jackknife samples\nshould agree with samples from a full jackknife analysis up to O(1/N).
    • \n
    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sqrt": {"fullname": "pyerrors.obs.Obs.sqrt", "modulename": "pyerrors.obs", "qualname": "Obs.sqrt", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.log": {"fullname": "pyerrors.obs.Obs.log", "modulename": "pyerrors.obs", "qualname": "Obs.log", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.exp": {"fullname": "pyerrors.obs.Obs.exp", "modulename": "pyerrors.obs", "qualname": "Obs.exp", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sin": {"fullname": "pyerrors.obs.Obs.sin", "modulename": "pyerrors.obs", "qualname": "Obs.sin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cos": {"fullname": "pyerrors.obs.Obs.cos", "modulename": "pyerrors.obs", "qualname": "Obs.cos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tan": {"fullname": "pyerrors.obs.Obs.tan", "modulename": "pyerrors.obs", "qualname": "Obs.tan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsin": {"fullname": "pyerrors.obs.Obs.arcsin", "modulename": "pyerrors.obs", "qualname": "Obs.arcsin", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccos": {"fullname": "pyerrors.obs.Obs.arccos", "modulename": "pyerrors.obs", "qualname": "Obs.arccos", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctan": {"fullname": "pyerrors.obs.Obs.arctan", "modulename": "pyerrors.obs", "qualname": "Obs.arctan", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.sinh": {"fullname": "pyerrors.obs.Obs.sinh", "modulename": "pyerrors.obs", "qualname": "Obs.sinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.cosh": {"fullname": "pyerrors.obs.Obs.cosh", "modulename": "pyerrors.obs", "qualname": "Obs.cosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.tanh": {"fullname": "pyerrors.obs.Obs.tanh", "modulename": "pyerrors.obs", "qualname": "Obs.tanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arcsinh": {"fullname": "pyerrors.obs.Obs.arcsinh", "modulename": "pyerrors.obs", "qualname": "Obs.arcsinh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arccosh": {"fullname": "pyerrors.obs.Obs.arccosh", "modulename": "pyerrors.obs", "qualname": "Obs.arccosh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.Obs.arctanh": {"fullname": "pyerrors.obs.Obs.arctanh", "modulename": "pyerrors.obs", "qualname": "Obs.arctanh", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs": {"fullname": "pyerrors.obs.CObs", "modulename": "pyerrors.obs", "qualname": "CObs", "kind": "class", "doc": "

    Class for a complex valued observable.

    \n"}, "pyerrors.obs.CObs.__init__": {"fullname": "pyerrors.obs.CObs.__init__", "modulename": "pyerrors.obs", "qualname": "CObs.__init__", "kind": "function", "doc": "

    \n", "signature": "(real, imag=0.0)"}, "pyerrors.obs.CObs.gamma_method": {"fullname": "pyerrors.obs.CObs.gamma_method", "modulename": "pyerrors.obs", "qualname": "CObs.gamma_method", "kind": "function", "doc": "

    Executes the gamma_method for the real and the imaginary part.

    \n", "signature": "(self, **kwargs):", "funcdef": "def"}, "pyerrors.obs.CObs.is_zero": {"fullname": "pyerrors.obs.CObs.is_zero", "modulename": "pyerrors.obs", "qualname": "CObs.is_zero", "kind": "function", "doc": "

    Checks whether both real and imaginary part are zero within machine precision.

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.CObs.conjugate": {"fullname": "pyerrors.obs.CObs.conjugate", "modulename": "pyerrors.obs", "qualname": "CObs.conjugate", "kind": "function", "doc": "

    \n", "signature": "(self):", "funcdef": "def"}, "pyerrors.obs.derived_observable": {"fullname": "pyerrors.obs.derived_observable", "modulename": "pyerrors.obs", "qualname": "derived_observable", "kind": "function", "doc": "

    Construct a derived Obs according to func(data, **kwargs) using automatic differentiation.

    \n\n
    Parameters
    \n\n
      \n
    • func (object):\narbitrary function of the form func(data, **kwargs). For the\nautomatic differentiation to work, all numpy functions have to have\nthe autograd wrapper (use 'import autograd.numpy as anp').
    • \n
    • data (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
    • \n
    • num_grad (bool):\nif True, numerical derivatives are used instead of autograd\n(default False). To control the numerical differentiation the\nkwargs of numdifftools.step_generators.MaxStepGenerator\ncan be used.
    • \n
    • man_grad (list):\nmanually supply a list or an array which contains the jacobian\nof func. Use cautiously, supplying the wrong derivative will\nnot be intercepted.
    • \n
    \n\n
    Notes
    \n\n

    For simple mathematical operations it can be practical to use anonymous\nfunctions. For the ratio of two observables one can e.g. use

    \n\n

    new_obs = derived_observable(lambda x: x[0] / x[1], [obs1, obs2])

    \n", "signature": "(func, data, array_mode=False, **kwargs):", "funcdef": "def"}, "pyerrors.obs.reweight": {"fullname": "pyerrors.obs.reweight", "modulename": "pyerrors.obs", "qualname": "reweight", "kind": "function", "doc": "

    Reweight a list of observables.

    \n\n
    Parameters
    \n\n
      \n
    • weight (Obs):\nReweighting factor. An Observable that has to be defined on a superset of the\nconfigurations in obs[i].idl for all i.
    • \n
    • obs (list):\nlist of Obs, e.g. [obs1, obs2, obs3].
    • \n
    • all_configs (bool):\nif True, the reweighted observables are normalized by the average of\nthe reweighting factor on all configurations in weight.idl and not\non the configurations in obs[i].idl. Default False.
    • \n
    \n", "signature": "(weight, obs, **kwargs):", "funcdef": "def"}, "pyerrors.obs.correlate": {"fullname": "pyerrors.obs.correlate", "modulename": "pyerrors.obs", "qualname": "correlate", "kind": "function", "doc": "

    Correlate two observables.

    \n\n
    Parameters
    \n\n
      \n
    • obs_a (Obs):\nFirst observable
    • \n
    • obs_b (Obs):\nSecond observable
    • \n
    \n\n
    Notes
    \n\n

    Keep in mind to only correlate primary observables which have not been reweighted\nyet. The reweighting has to be applied after correlating the observables.\nCurrently only works if ensembles are identical (this is not strictly necessary).

    \n", "signature": "(obs_a, obs_b):", "funcdef": "def"}, "pyerrors.obs.covariance": {"fullname": "pyerrors.obs.covariance", "modulename": "pyerrors.obs", "qualname": "covariance", "kind": "function", "doc": "

    Calculates the error covariance matrix of a set of observables.

    \n\n

    WARNING: This function should be used with care, especially for observables with support on multiple\n ensembles with differing autocorrelations. See the notes below for details.

    \n\n

    The gamma method has to be applied first to all observables.

    \n\n
    Parameters
    \n\n
      \n
    • obs (list or numpy.ndarray):\nList or one dimensional array of Obs
    • \n
    • visualize (bool):\nIf True plots the corresponding normalized correlation matrix (default False).
    • \n
    • correlation (bool):\nIf True the correlation matrix instead of the error covariance matrix is returned (default False).
    • \n
    • smooth (None or int):\nIf smooth is an integer 'E' between 2 and the dimension of the matrix minus 1 the eigenvalue\nsmoothing procedure of hep-lat/9412087 is applied to the correlation matrix which leaves the\nlargest E eigenvalues essentially unchanged and smoothes the smaller eigenvalues to avoid extremely\nsmall ones.
    • \n
    \n\n
    Notes
    \n\n

    The error covariance is defined such that it agrees with the squared standard error for two identical observables\n$$\\operatorname{cov}(a,a)=\\sum_{s=1}^N\\delta_a^s\\delta_a^s/N^2=\\Gamma_{aa}(0)/N=\\operatorname{var}(a)/N=\\sigma_a^2$$\nin the absence of autocorrelation.\nThe error covariance is estimated by calculating the correlation matrix assuming no autocorrelation and then rescaling the correlation matrix by the full errors including the previous gamma method estimate for the autocorrelation of the observables. The covariance at windowsize 0 is guaranteed to be positive semi-definite\n$$\\sum_{i,j}v_i\\Gamma_{ij}(0)v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i,j}v_i\\delta_i^s\\delta_j^s v_j=\\frac{1}{N}\\sum_{s=1}^N\\sum_{i}|v_i\\delta_i^s|^2\\geq 0\\,,$$ for every $v\\in\\mathbb{R}^M$, while such an identity does not hold for larger windows/lags.\nFor observables defined on a single ensemble our approximation is equivalent to assuming that the integrated autocorrelation time of an off-diagonal element is equal to the geometric mean of the integrated autocorrelation times of the corresponding diagonal elements.\n$$\\tau_{\\mathrm{int}, ij}=\\sqrt{\\tau_{\\mathrm{int}, i}\\times \\tau_{\\mathrm{int}, j}}$$\nThis construction ensures that the estimated covariance matrix is positive semi-definite (up to numerical rounding errors).

    \n", "signature": "(obs, visualize=False, correlation=False, smooth=None, **kwargs):", "funcdef": "def"}, "pyerrors.obs.import_jackknife": {"fullname": "pyerrors.obs.import_jackknife", "modulename": "pyerrors.obs", "qualname": "import_jackknife", "kind": "function", "doc": "

    Imports jackknife samples and returns an Obs

    \n\n
    Parameters
    \n\n
      \n
    • jacks (numpy.ndarray):\nnumpy array containing the mean value as zeroth entry and\nthe N jackknife samples as first to Nth entry.
    • \n
    • name (str):\nname of the ensemble the samples are defined on.
    • \n
    \n", "signature": "(jacks, name, idl=None):", "funcdef": "def"}, "pyerrors.obs.merge_obs": {"fullname": "pyerrors.obs.merge_obs", "modulename": "pyerrors.obs", "qualname": "merge_obs", "kind": "function", "doc": "

    Combine all observables in list_of_obs into one new observable

    \n\n
    Parameters
    \n\n
      \n
    • list_of_obs (list):\nlist of the Obs object to be combined
    • \n
    \n\n
    Notes
    \n\n

    It is not possible to combine obs which are based on the same replicum

    \n", "signature": "(list_of_obs):", "funcdef": "def"}, "pyerrors.obs.cov_Obs": {"fullname": "pyerrors.obs.cov_Obs", "modulename": "pyerrors.obs", "qualname": "cov_Obs", "kind": "function", "doc": "

    Create an Obs based on mean(s) and a covariance matrix

    \n\n
    Parameters
    \n\n
      \n
    • mean (list of floats or float):\nN mean value(s) of the new Obs
    • \n
    • cov (list or array):\n2d (NxN) Covariance matrix, 1d diagonal entries or 0d covariance
    • \n
    • name (str):\nidentifier for the covariance matrix
    • \n
    • grad (list or array):\nGradient of the Covobs wrt. the means belonging to cov.
    • \n
    \n", "signature": "(means, cov, name, grad=None):", "funcdef": "def"}, "pyerrors.roots": {"fullname": "pyerrors.roots", "modulename": "pyerrors.roots", "kind": "module", "doc": "

    \n"}, "pyerrors.roots.find_root": {"fullname": "pyerrors.roots.find_root", "modulename": "pyerrors.roots", "qualname": "find_root", "kind": "function", "doc": "

    Finds the root of the function func(x, d) where d is an Obs.

    \n\n
    Parameters
    \n\n
      \n
    • d (Obs):\nObs passed to the function.
    • \n
    • func (object):\nFunction to be minimized. Any numpy functions have to use the autograd.numpy wrapper.\nExample:

      \n\n
      \n
      import autograd.numpy as anp\ndef root_func(x, d):\n   return anp.exp(-x ** 2) - d\n
      \n
    • \n
    • guess (float):\nInitial guess for the minimization.

    • \n
    \n\n
    Returns
    \n\n
      \n
    • res (Obs):\nObs valued root of the function.
    • \n
    \n", "signature": "(d, func, guess=1.0, **kwargs):", "funcdef": "def"}, "pyerrors.version": {"fullname": "pyerrors.version", "modulename": "pyerrors.version", "kind": "module", "doc": "

    \n"}}, "docInfo": {"pyerrors": {"qualname": 0, "fullname": 1, "annotation": 0, "default_value": 0, "signature": 0, "bases": 0, "doc": 8258}, "pyerrors.correlators": {"qualname": 0, "fullname": 2, "annotation": 0, "default_value": 0, "signature": 0, "bases": 0, "doc": 3}, "pyerrors.correlators.Corr": {"qualname": 1, "fullname": 3, "annotation": 0, "default_value": 0, "signature": 0, "bases": 0, "doc": 108}, "pyerrors.correlators.Corr.__init__": {"qualname": 3, "fullname": 5, "annotation": 0, "default_value": 0, "signature": 40, "bases": 0, "doc": 94}, "pyerrors.correlators.Corr.gamma_method": {"qualname": 3, "fullname": 5, "annotation": 0, "default_value": 0, "signature": 18, "bases": 0, "doc": 13}, "pyerrors.correlators.Corr.gm": {"qualname": 2, "fullname": 4, "annotation": 0, "default_value": 0, "signature": 18, "bases": 0, "doc": 13}, "pyerrors.correlators.Corr.projected": {"qualname": 2, "fullname": 4, "annotation": 0, "default_value": 0, "signature": 43, "bases": 0, "doc": 64}, 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