Converters¶
Wien2k Converter¶
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class
triqs_dft_tools.converters.wien2k_converter.
Wien2kConverter
(filename, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', parproj_subgrp='dft_parproj_input', symmpar_subgrp='dft_symmpar_input', bands_subgrp='dft_bands_input', misc_subgrp='dft_misc_input', transp_subgrp='dft_transp_input', repacking=False)[source]¶ Bases:
triqs_dft_tools.converters.converter_tools.ConverterTools
Conversion from Wien2k output to an hdf5 file that can be used as input for the SumkDFT class.
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__init__
(filename, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', parproj_subgrp='dft_parproj_input', symmpar_subgrp='dft_symmpar_input', bands_subgrp='dft_bands_input', misc_subgrp='dft_misc_input', transp_subgrp='dft_transp_input', repacking=False)[source]¶ Initialise the class.
Parameters: filename : string
Base name of DFT files.
hdf_filename : string, optional
Name of hdf5 archive to be created.
dft_subgrp : string, optional
Name of subgroup storing necessary DFT data.
symmcorr_subgrp : string, optional
Name of subgroup storing correlated-shell symmetry data.
parproj_subgrp : string, optional
Name of subgroup storing partial projector data.
symmpar_subgrp : string, optional
Name of subgroup storing partial-projector symmetry data.
bands_subgrp : string, optional
Name of subgroup storing band data.
misc_subgrp : string, optional
Name of subgroup storing miscellaneous DFT data.
transp_subgrp : string, optional
Name of subgroup storing transport data.
repacking : boolean, optional
Does the hdf5 archive need to be repacked to save space?
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convert_bands_input
()[source]¶ Reads the appropriate files and stores the data for the bands_subgrp in the hdf5 archive.
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convert_dft_input
()[source]¶ Reads the appropriate files and stores the data for the
- dft_subgrp
- symmcorr_subgrp
- misc_subgrp
in the hdf5 archive.
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convert_misc_input
()[source]¶ Reads additional information on:
- the band window from
case.oubwin
, - lattice parameters from
case.struct
, - symmetries from
case.outputs
,
if those Wien2k files are present and stores the data in the hdf5 archive. This function is automatically called by
convert_dft_input
.- the band window from
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convert_parproj_input
()[source]¶ Reads the appropriate files and stores the data for the
- parproj_subgrp
- symmpar_subgrp
in the hdf5 archive.
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convert_symmetry_input
(orbits, symm_file, symm_subgrp, SO, SP)[source]¶ Reads and stores symmetrisation data from symm_file, which can be is case.sympar or case.symqmc.
Parameters: orbits : list of dicts
This is either shells or corr_shells depending on whether the symmetry information is for correlated shells or partial projectors.
symm_file : string
Name of the file containing symmetry data. This is case.symqmc for correlated shells and case.sympar for partial projectors.
symm_subgrp : string, optional
Name of subgroup storing symmetry data.
SO : integer
Is spin-orbit coupling considered?
SP : integer
Is the system spin-polarised?
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H(k) Converter¶
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class
triqs_dft_tools.converters.hk_converter.
HkConverter
(filename, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', repacking=False)[source]¶ Conversion from general H(k) file to an hdf5 file that can be used as input for the SumKDFT class.
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__init__
(filename, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', repacking=False)[source]¶ Initialise the class.
Parameters: filename : string
Name of file containing the H(k) and other relevant data.
hdf_filename : string, optional
Name of hdf5 archive to be created.
dft_subgrp : string, optional
Name of subgroup storing necessary DFT data.
symmcorr_subgrp : string, optional
Name of subgroup storing correlated-shell symmetry data. The group is actually empty; it is just included for compatibility.
repacking : boolean, optional
Does the hdf5 archive need to be repacked to save space?
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convert_dft_input
(first_real_part_matrix=True, only_upper_triangle=False, weights_in_file=False)[source]¶ Reads the appropriate files and stores the data for the dft_subgrp in the hdf5 archive.
Parameters: first_real_part_matrix : boolean, optional
Should all the real components for given k be read in first, followed by the imaginary parts?
only_upper_triangle : boolean, optional
Should only the upper triangular part of H(k) be read in?
weights_in_file : boolean, optional
Are the k-point weights to be read in?
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Wannier90 Converter¶
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class
triqs_dft_tools.converters.wannier90_converter.
Wannier90Converter
(seedname, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', repacking=False)[source]¶ Conversion from Wannier90 output to an hdf5 file that can be used as input for the SumkDFT class.
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__init__
(seedname, hdf_filename=None, dft_subgrp='dft_input', symmcorr_subgrp='dft_symmcorr_input', repacking=False)[source]¶ Initialise the class.
Parameters: seedname : string
Base name of Wannier90 files
hdf_filename : string, optional
Name of hdf5 archive to be created
dft_subgrp : string, optional
Name of subgroup storing necessary DFT data
symmcorr_subgrp : string, optional
Name of subgroup storing correlated-shell symmetry data
repacking : boolean, optional
Does the hdf5 archive need to be repacked to save space?
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convert_dft_input
()[source]¶ Reads the appropriate files and stores the data for the
- dft_subgrp
- symmcorr_subgrp
in the hdf5 archive.
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find_rot_mat
(n_sh, sh_lst, sh_map, ham0)[source]¶ Method for finding the matrices that bring from local to global coordinate systems (and viceversa), based on the eigenvalues of H(R=0)
Parameters: n_sh : integer
number of shells
sh_lst : list of shells-type dictionaries
contains the shells (could be correlated or not)
sh_map : list of integers
mapping between shells
ham0 : numpy.array of floats
local Hamiltonian matrix elements
Returns: istatus : integer
if 0, something failed in the construction of the matrices
rot_mat : list of numpy.array
rotation matrix for each of the shell
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fourier_ham
(norb, h_of_r)[source]¶ Method for obtaining H(k) from H(R) via Fourier transform The R vectors and k-point mesh are read from global module variables
Parameters: norb : integer
number of orbitals
h_of_r : list of numpy.array[norb,norb]
Hamiltonian H(R) in Wannier basis
Returns: h_of_k : list of numpy.array[norb,norb]
transformed Hamiltonian H(k) in Wannier basis
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kmesh_build
(msize=None, mmode=0)[source]¶ Method for the generation of the k-point mesh. Right now it only supports the option for generating a full grid containing k=0,0,0.
Parameters: msize : list of 3 integers
the dimensions of the mesh
mmode : integer
mesh generation mode (right now, only full grid available)
Returns: nkpt : integer
total number of k-points in the mesh
k_mesh : numpy.array[nkpt,3] of floats
the coordinates of all k-points
wk : numpy.array[nkpt] of floats
the weight of each k-point
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read_wannier90hr
(hr_filename='wannier_hr.dat')[source]¶ Method for reading the seedname_hr.dat file produced by Wannier90 (http://wannier.org)
Parameters: hr_filename : string
full name of the H(R) file produced by Wannier90 (usually seedname_hr.dat)
Returns: nrpt : integer
number of R vectors found in the file
rvec_idx : numpy.array of integers
Miller indices of the R vectors
rvec_deg : numpy.array of floats
weight of the R vectors
num_wf : integer
number of Wannier functions found
h_of_r : list of numpy.array
<w_i|H(R)|w_j> = Hamilonian matrix elements in the Wannier basis
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Converter Tools¶
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class
triqs_dft_tools.converters.converter_tools.
ConverterTools
[source]¶ -
det_shell_equivalence
(corr_shells)[source]¶ Determine the equivalence of correlated shells.
Parameters: corr_shells : list of dicts
See documentation of necessary hdf5 elements.
Returns: n_inequiv_shells : integer
Number of inequivalent shells.
corr_to_inequiv : list
Mapping between correlated shell index and inequivalent shell index. corr_to_inequiv(i_corr_shells) = i_inequiv_shells
inequiv_to_corr : list
Mapping between inequivalent shell index and correlated shell index. inequiv_to_corr(i_inequiv_shells) = i_corr_shells
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