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stm_sts_from_wfn.py
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stm_sts_from_wfn.py
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#!/usr/bin/env python
import os
import numpy as np
import time
import copy
import sys
import argparse
ang_2_bohr = 1.0/0.52917721067
hart_2_ev = 27.21138602
import cp2k_spm_tools.cp2k_grid_orbitals as cgo
import cp2k_spm_tools.cp2k_stm_sts as css
from cp2k_spm_tools import common, cube_utils
from cp2k_spm_tools.cube import Cube
from mpi4py import MPI
comm = MPI.COMM_WORLD
mpi_rank = comm.Get_rank()
mpi_size = comm.Get_size()
parser = argparse.ArgumentParser(
description='Puts the CP2K orbitals on grid and calculates STM.')
### ----------------------------------------------------------------------
### Input and output files
parser.add_argument(
'--cp2k_input_file',
metavar='FILENAME',
required=True,
help='CP2K input of the SCF calculation.')
parser.add_argument(
'--basis_set_file',
metavar='FILENAME',
required=True,
help='File containing the used basis sets.')
parser.add_argument(
'--xyz_file',
metavar='FILENAME',
required=True,
help='.xyz file containing the geometry.')
parser.add_argument(
'--wfn_file',
metavar='FILENAME',
required=True,
help='Restart file containing the final wavefunction.')
parser.add_argument(
'--hartree_file',
metavar='FILENAME',
required=True,
help='Cube file containing the hartree potential.')
parser.add_argument(
'--output_file',
metavar='FILENAME',
default="./stm.npz",
help='File, where to save the STM/STS output')
parser.add_argument(
'--orb_output_file',
metavar='FILENAME',
default="./orb.npz",
help='File, where to save the orbital output')
### ----------------------------------------------------------------------
### Parameters for putting orbitals on grid
parser.add_argument(
'--eval_region',
type=str,
nargs=6,
metavar='X',
required=True,
help=common.eval_region_description
)
parser.add_argument(
'--dx',
type=float,
metavar='DX',
required=True,
help='Spatial step for the grid (angstroms).')
parser.add_argument(
'--eval_cutoff',
type=float,
metavar='D',
default=16.0,
help=("Size of the region around the atom where each"
" orbital is evaluated (only used for 'G' region).")
)
parser.add_argument(
'--extrap_extent',
type=float,
metavar='H',
default=4.0,
required=True,
help="The extent of the extrapolation region. (angstrom)"
)
### ----------------------------------------------------------------------
### Gas phase analysis parameters - image at orbital energies
parser.add_argument(
'--n_homo',
type=int,
metavar='N',
default=0,
help="Number of HOMO orbitals to analyse.")
parser.add_argument(
'--n_lumo',
type=int,
metavar='N',
default=0,
help="Number of LUMO orbitals to analyse.")
parser.add_argument(
'--orb_heights',
nargs='*',
type=float,
metavar='H',
help="List of heights for constant height orbital pictures (wrt topmost atom).")
parser.add_argument(
'--orb_isovalues',
nargs='*',
type=float,
metavar='C',
help="List of charge density isovalues for constant current orbital pictures")
parser.add_argument(
'--orb_fwhms',
nargs='*',
type=float,
default=[0.02],
help="Full width at half maximum for orbital STS gaussian broadening. (eV)")
### ----------------------------------------------------------------------
### Slab system analysis parameters - images at specified energies
###
### Option 1: continuous selection
parser.add_argument(
'--energy_range',
nargs=3,
type=float,
metavar='E',
help='Selection of STM/STS energy values based on a range: min, max and differential.')
###
### Option 2: discrete selection
parser.add_argument(
'--energies',
nargs='*',
type=float,
metavar='E',
help='Discrete energies where to run the STM/STS.')
### ----------------------------------------------------------------------
### Parameters for STM/STS series
parser.add_argument(
'--heights',
nargs='*',
type=float,
metavar='H',
help="List of heights for constant height STM pictures (wrt topmost atom).")
parser.add_argument(
'--isovalues',
nargs='*',
type=float,
metavar='C',
help="List of charge density isovalues for constant current STM pictures.")
parser.add_argument(
'--fwhms',
nargs='*',
type=float,
default=[0.1],
help="Full width at half maximum for STS gaussian broadening. (eV)")
### ----------------------------------------------------------------------
### P - tip ratio list
parser.add_argument(
'--p_tip_ratios',
nargs='+',
type=float,
metavar='P',
default=[0.0],
help=("List of p character of the STM tip: 0.0 corresponds"
"to fully s-type and 1.0 to fully p-type tip")
)
### ----------------------------------------------------------------------
time0 = time.time()
### ------------------------------------------------------
### Parse args for only one rank to suppress duplicate stdio
### ------------------------------------------------------
args = None
args_success = False
try:
if mpi_rank == 0:
args = parser.parse_args()
args_success = True
finally:
args_success = comm.bcast(args_success, root=0)
if not args_success:
print(mpi_rank, "exiting")
exit(0)
args = comm.bcast(args, root=0)
### ------------------------------------------------------
### Energy values for STM/STS
### ------------------------------------------------------
if args.energies is not None:
e_arr = np.array(args.energies)
elif args.energy_range is not None:
emin, emax, de = args.energy_range
e_arr = np.arange(emin, emax+de/2, de)
else:
e_arr = None
max_fwhm = np.max(args.fwhms)
if e_arr is not None:
sel_emin = np.min(e_arr) - 2.0*max_fwhm
sel_emax = np.max(e_arr) + 2.0*max_fwhm
else:
sel_emin = None
sel_emax = None
### ------------------------------------------------------
### Evaluate orbitals on the real-space grid
### ------------------------------------------------------
cp2k_grid_orb = cgo.Cp2kGridOrbitals(mpi_rank, mpi_size, mpi_comm=comm, single_precision=True)
cp2k_grid_orb.read_cp2k_input(args.cp2k_input_file)
cp2k_grid_orb.read_xyz(args.xyz_file)
cp2k_grid_orb.center_atoms_to_cell()
cp2k_grid_orb.read_basis_functions(args.basis_set_file)
cp2k_grid_orb.load_restart_wfn_file(args.wfn_file,
emin=sel_emin, emax=sel_emax,
n_occ=args.n_homo, n_virt=args.n_lumo
)
print("R%d/%d: loaded wfn, %.2fs"%(mpi_rank, mpi_size, (time.time() - time0)))
sys.stdout.flush()
time1 = time.time()
eval_reg = common.parse_eval_region_input(args.eval_region, cp2k_grid_orb.ase_atoms, cp2k_grid_orb.cell)
# --------
# Make sure extrap extent is compatible with heights
atoms_max_z = np.max(cp2k_grid_orb.ase_atoms.positions[:, 2])
eval_z_above_atoms = eval_reg[2][1] - atoms_max_z
extrap_extent = args.extrap_extent
for hs in [args.orb_heights, args.heights]:
if hs is not None:
if np.max(hs) - eval_z_above_atoms > extrap_extent:
print("Increasing extrap. extent to be compatible with heights.")
extrap_extent = np.max(hs)- eval_z_above_atoms
# --------
cp2k_grid_orb.calc_morbs_in_region(args.dx,
x_eval_region = eval_reg[0],
y_eval_region = eval_reg[1],
z_eval_region = eval_reg[2],
pbc = (True, True, False),
reserve_extrap = extrap_extent,
eval_cutoff = args.eval_cutoff)
print("R%d/%d: evaluated wfn, %.2fs"%(mpi_rank, mpi_size, (time.time() - time1)))
sys.stdout.flush()
time1 = time.time()
### ------------------------------------------------------
### Extrapolate orbitals
### ------------------------------------------------------
hart_cube = Cube()
hart_cube.read_cube_file(args.hartree_file)
extrap_plane_z = eval_reg[2][1] / ang_2_bohr - np.max(cp2k_grid_orb.ase_atoms.positions[:, 2])
hart_plane = hart_cube.get_plane_above_topmost_atom(extrap_plane_z) - cp2k_grid_orb.ref_energy/hart_2_ev
cp2k_grid_orb.extrapolate_morbs(hart_plane=hart_plane)
print("R%d/%d: extrapolated wfn, %.2fs"%(mpi_rank, mpi_size, (time.time() - time1)))
sys.stdout.flush()
time1 = time.time()
### ------------------------------------------------------
### Calculate the ionization potential (just for output)
### ------------------------------------------------------
if mpi_rank == 0:
# NB: currently only accurate for isolated molecules
if cp2k_grid_orb.nspin == 1:
homo_en = cp2k_grid_orb.global_morb_energies[0][cp2k_grid_orb.i_homo_glob[0]]
else:
homo_en = np.max([
cp2k_grid_orb.global_morb_energies[0][cp2k_grid_orb.i_homo_glob[0]],
cp2k_grid_orb.global_morb_energies[1][cp2k_grid_orb.i_homo_glob[1]]
])
ion_pot = cube_utils.find_vacuum_level_naive(hart_cube) - (homo_en + cp2k_grid_orb.ref_energy)
print("IONIZATION POTENIAL (eV): %.6f (accurate only for isolated molecules)" % ion_pot)
sys.stdout.flush()
### ------------------------------------------------------
### Set up STM object
### ------------------------------------------------------
stm = css.STM(mpi_comm = comm, cp2k_grid_orb = cp2k_grid_orb, p_tip_ratios = args.p_tip_ratios)
stm.gather_global_energies()
stm.divide_by_space()
### ------------------------------------------------------
### Run STM-STS analysis for orbitals
### ------------------------------------------------------
orb_heights = args.orb_heights if args.orb_heights is not None else []
orb_isovalues = args.orb_isovalues if args.orb_isovalues is not None else []
orb_fwhms = args.orb_fwhms if args.orb_fwhms is not None else []
if len(orb_fwhms) != 0 and (len(orb_heights) != 0 or len(orb_isovalues) != 0):
orbital_list = list(range(-args.n_homo + 1, args.n_lumo + 1))
stm.create_orb_series(orbital_list, orb_heights, orb_isovalues, orb_fwhms)
stm.collect_and_save_orb_maps(path=args.orb_output_file)
### ------------------------------------------------------
### Run STM-STS analysis for general energies
### ------------------------------------------------------
heights = args.heights if args.heights is not None else []
isovalues = args.isovalues if args.isovalues is not None else []
fwhms = args.fwhms if args.fwhms is not None else []
if e_arr is not None and len(fwhms) != 0 and (len(heights) != 0 or len(isovalues) != 0):
stm.calculate_stm_maps(fwhms, isovalues, heights, e_arr)
stm.collect_and_save_stm_maps(path=args.output_file)
print("R%d/%d: finished, total time: %.2fs"%(mpi_rank, mpi_size, (time.time() - time0)))