*** FILE AUTOMATICALLY CREATED: DO NOT EDIT, CHANGES WILL BE LOST *** ------------------------------------------------------------------------ INPUT FILE DESCRIPTION Program: bgw2pw.x / PWscf / Quantum Espresso (version: 6.1) ------------------------------------------------------------------------ Purpose of bgw2pw.x: Converts BerkeleyGW WFN and RHO files to the format of pw.x. This can be useful, for example, if you generate the plane waves on top of the valence bands and want to diagonalize them in pw.x. Look at the documentation for SAPO code in BerkeleyGW for more information. bgw2pw.x reads common parameters from file "prefix".save/data-file.xml and writes files "prefix".save/charge-density.dat (charge density in R-space), "prefix".save/gvectors.dat (G-vectors for charge density and potential), "prefix".save/K$n/eigenval.xml (eigenvalues and occupations for nth k-point), "prefix".save/K$n/evc.dat (wavefunctions in G-space for nth k-point), and "prefix".save/K$n/gkvectors.dat (G-vectors for nth k-point). bgw2pw.x doesn't modify file "prefix".save/data-file.xml so make changes to this file manually (for example, you will need to change the number of bands if you are using bgw2pw.x in conjunction with SAPO code in BerkeleyGW). Structure of the input data: ============================ &INPUT_BGW2PW ... / ======================================================================== NAMELIST: &INPUT_BGW2PW +-------------------------------------------------------------------- Variable: prefix Type: STRING Status: MANDATORY Description: prefix of files saved by program pw.x +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: outdir Type: STRING Default: './' Description: the scratch directory where the massive data-files are written +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: real_or_complex Type: INTEGER Default: 2 Description: 1 | 2 1 for real flavor of BerkeleyGW (for systems with inversion symmetry and time-reversal symmetry) or 2 for complex flavor of BerkeleyGW (for systems without inversion symmetry and time-reversal symmetry) +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: wfng_flag Type: LOGICAL Default: .FALSE. Description: read wavefunctions in G-space from BerkeleyGW WFN file +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: wfng_file Type: STRING Default: 'WFN' Description: name of BerkeleyGW WFN input file. Not used if "wfng_flag" = .FALSE. +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: wfng_nband Type: INTEGER Default: 0 Description: number of bands to write (0 = all). Not used if "wfng_flag" = .FALSE. +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: rhog_flag Type: LOGICAL Default: .FALSE. Description: read charge density in G-space from BerkeleyGW RHO file +-------------------------------------------------------------------- +-------------------------------------------------------------------- Variable: rhog_file Type: STRING Default: 'RHO' Description: name of BerkeleyGW RHO input file. Not used if "rhog_flag" = .FALSE. +-------------------------------------------------------------------- ===END OF NAMELIST====================================================== This file has been created by helpdoc utility on Fri Mar 03 06:56:20 UTC 2017