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gawk | ||
vim | ||
nano | ||
mc |
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name: ci | ||
on: | ||
push: | ||
branches: | ||
- master | ||
jobs: | ||
deploy: | ||
runs-on: ubuntu-latest | ||
steps: | ||
- uses: actions/checkout@v2 | ||
- uses: actions/setup-python@v2 | ||
with: | ||
python-version: 3.x | ||
- run: pip install mkdocs-material | ||
- run: mkdocs gh-deploy --force |
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# .readthedocs.yml | ||
# Read the Docs configuration file | ||
# See https://docs.readthedocs.io/en/stable/config-file/v2.html for details | ||
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# Required | ||
version: 2 | ||
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# Build documentation in the docs/ directory with Sphinx | ||
sphinx: | ||
configuration: doc/conf.py | ||
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# Build documentation with MkDocs | ||
#mkdocs: | ||
# configuration: mkdocs.yml | ||
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# Optionally build your docs in additional formats such as PDF and ePub | ||
formats: all | ||
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# Optionally set the version of Python and requirements required to build your docs | ||
python: | ||
version: 3.7 | ||
install: | ||
- requirements: doc/requirements.txt |
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gold 1 1986 USA American Eagle | ||
gold 1 1908 Austria-Hungary Franz Josef 100 Korona | ||
silver 10 1981 USA ingot | ||
gold 1 1984 Switzerland ingot | ||
gold 1 1979 RSA Krugerrand | ||
gold 0.5 1981 RSA Krugerrand | ||
gold 0.1 1986 PRC Panda | ||
silver 1 1986 USA Liberty dollar | ||
gold 0.25 1986 USA Liberty 5-dollar piece | ||
silver 0.5 1986 USA Liberty 50-cent piece | ||
silver 1 1987 USA Constitution dollar | ||
gold 0.25 1987 USA Constitution 5-dollar piece | ||
gold 1 1988 Canada Maple Leaf |
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#!/usr/bin/awk -f | ||
{ | ||
country[$4]++ | ||
} | ||
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END { | ||
for (i in country) print "Country: " i," count: ", country[i] | ||
} |
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1 2 3 | ||
4 5 6 | ||
7 8 9 10 text |
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#!/usr/bin/awk -f | ||
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BEGIN { AU2eV= 27.211383 } | ||
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/Distance matrix/ {getline; getline; getline; getline; getline; getline; rOH= $5} | ||
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/Counterpoise: corrected energy/ { printf "%.12f %.6f\n", rOH, $5*AU2eV } |
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#!/usr/bin/awk -f | ||
# x,y,z in Angstroms | ||
NR > 2 { | ||
mx= mx + $2*$5; my= my + $3*$5; mz= mz + $4*$5; | ||
} | ||
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END { | ||
norm=sqrt(mx**2+my**2+mz**2); | ||
# Convert to Debye | ||
toD= 4.80320425; | ||
mx= mx*toD; my= my*toD; mz= mz*toD; | ||
norm= norm*toD; | ||
printf("Dipole Moment\t x\t\t y\t\t z\t\t| D.Moment |\n"); | ||
printf(" [ Debye ] \t%f\t%f\t%f\t%f\n", mx, my, mz, norm); | ||
} |
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7 | ||
Wannier centres, written by Wannier90 on 6Aug2013 at 14:23:10 | ||
X 6.50000026 6.18706578 6.50000000 -2 | ||
X 6.50000000 6.71337672 6.50000002 -2 | ||
X 6.50000008 6.95339960 6.49999998 -2 | ||
X 6.49999971 6.54636884 6.50000000 -2 | ||
H 6.50000000 7.09480000 7.26880000 1 | ||
H 6.50000000 7.09480000 5.73120000 1 | ||
O 6.50000000 6.50000000 6.50000000 6 |
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Daniel 10 | ||
Anders 7 | ||
Sven 56 | ||
Ali 17 | ||
Peter 6 |
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Peter Monday | ||
Sven Sunday | ||
David Tuesday |
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#!/usr/bin/awk -f | ||
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{ | ||
names[$1]= 1; | ||
data[$1,ARGIND]= $2 | ||
} | ||
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END{ | ||
for (i in names) print i"\t\t"data[i,1]"\t\t"data[i,2] | ||
} |
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# Anharm harm | ||
2858.351 3173.516 | ||
2797.693 3131.408 | ||
2682.453 3019.173 | ||
2710.734 3056.025 | ||
2989.402 3273.493 | ||
2558.539 2919.306 | ||
2781.281 3111.231 | ||
2707.999 3052.427 | ||
2575.868 2934.403 | ||
2784.882 3111.663 | ||
2977.694 3266.289 | ||
2652.853 2993.294 | ||
2868.582 3163.679 | ||
3076.485 3334.419 | ||
2883.267 3188.332 | ||
3137.228 3389.384 | ||
3425.697 3615.290 | ||
3094.083 3356.917 |
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#!/usr/bin/awk -f | ||
BEGIN{ | ||
FWHM=30; # Default smearing if none is provided on the command line | ||
FWHM= FWHM/2.35482 | ||
# trick to read parameters from the command line | ||
if (ARGC==3) FWHM=ARGV[2]; ARGC=2; | ||
} | ||
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!/#/ { | ||
f++; | ||
if (f==1) {fmin=$1; fmax=$1} | ||
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freq[f]=$1; | ||
if (fmin > $1) fmin=$1; | ||
if (fmax < $1) fmax=$1; | ||
nfreq=f; | ||
} | ||
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END{ | ||
print "# freq intensity | nfreq: "nfreq" fmin: "fmin" fmax: "fmax | ||
for (i=int(fmin -5*FWHM); i<=int(fmax +5*FWHM);i++){ | ||
for (f=1;f<=nfreq;f++){ | ||
data[i]= data[i] + gauss(freq[f],i,FWHM); | ||
} | ||
print i,data[i] | ||
} | ||
} | ||
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function gauss(x0,x,c){ | ||
area=1; | ||
if ((x-x0)**2 < 10000) { return area*exp(-(((x-x0))**2)/(2.*c**2))} | ||
else {return 0.0} | ||
} |
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#!/usr/bin/gnuplot | ||
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set term pngcairo size 800, 400 enhanced | ||
set out "Gauss-smearing.png" | ||
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set border | ||
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set key top left | ||
set title "Gaussian smearing with FWHM 10 and 30" | ||
set xlabel "Frequency" | ||
set ylabel "Intensity" | ||
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plot "< ./gauss-smear-data.awk freq.dat 30" u ($1 ):($2) w l t "Gauss smearing 30" lw 2,\ | ||
"< ./gauss-smear-data.awk freq.dat 10" u ($1 ):($2) w l t "Gauss smearing 10" lw 2,\ | ||
"freq.dat" u ($1):(1) w impulses t "" lc rgb "blue" | ||
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!display Gauss-smearing.png |
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#!/usr/bin/awk -f | ||
BEGIN{ | ||
cmd1= "bzcat "ARGV[1]; | ||
cmd2= "bzcat "ARGV[2]; | ||
cmd3= "bzcat "ARGV[3]; | ||
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NF=1; while(NF>0){ cmd2 |& getline; } cmd2 |& getline; | ||
NF=1; while(NF>0){ cmd3 |& getline; } cmd3 |& getline; | ||
NF=1; while(NF>0){ cmd1 |& getline; print } cmd1 |& getline; print; | ||
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do { | ||
cmd1 |& getline; split($0,d1) | ||
cmd2 |& getline; split($0,d2) | ||
cmd3 |& getline; split($0,d3) | ||
for(i=1;i<=NF;i++) printf "%18.11e ", d1[i]-d2[i]-d3[i] | ||
print"" | ||
} while ($1*1==$1) | ||
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} | ||
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#!/usr/bin/env python | ||
# Author: Pavlin Mitev | ||
# version 2015.10.22 | ||
import numpy as np | ||
import os,sys,time | ||
from math import sin, cos, degrees, radians | ||
from ase import Atoms | ||
from ase.calculators.vasp import VaspChargeDensity | ||
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import scipy.ndimage as ndimage | ||
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import matplotlib.pyplot as plt | ||
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#import scipy.interpolate as interpolate | ||
#from scipy.interpolate import griddata | ||
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#====================================== | ||
atom1= 2 # atom in the center | ||
atom2= 1 # atom from the plane | ||
atom3= 0 # second atom in the plain | ||
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npx= 90 # number of point to sample the plane in x | ||
npy= 90 # number of point to sample the plane in y | ||
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angle= radians(-144) # rotate the final plot around the central atom | ||
#angle= radians(0) | ||
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start= time.time() | ||
sys.stdout.write("Reading CHGCAR... "); sys.stdout.flush() | ||
CHGCAR= VaspChargeDensity("CHGCAR") | ||
end= time.time() | ||
print "finished. {0}".format(end-start) | ||
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cell= CHGCAR.atoms[0].cell | ||
nx,ny,nz= np.shape(CHGCAR.chg[0]) | ||
ncell= cell/np.array([nx,ny,nz]) | ||
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# define plane ================================= | ||
p1= CHGCAR.atoms[0].get_scaled_positions()[atom1] | ||
p2= CHGCAR.atoms[0].get_scaled_positions()[atom2] | ||
p3= CHGCAR.atoms[0].get_scaled_positions()[atom3] | ||
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# get normal to the plane | ||
v1= p2-p1; | ||
v2= p3-p1; | ||
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v1n= np.dot(v1,cell); # v1 in Cartesian | ||
v2n= np.dot(v2,cell); # v2 in Cartesian | ||
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v1n= v1n/np.linalg.norm(v1n) # v1 unit in Cartesian | ||
v2n= v2n/np.linalg.norm(v2n) # v2 unit in Cartesian | ||
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vnorm= np.cross(v1n,v2n); | ||
vnorm= vnorm/np.linalg.norm(vnorm) | ||
#vnorm= np.dot(vnorm,cell) # vnorm in Cartesian | ||
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# Rotate the plane ============================== | ||
axis = vnorm; | ||
axis_skewed = [ [0, -axis[2], axis[1]], [ axis[2], 0, -axis[0] ] , [ -axis[1], axis[0], 0] ]; | ||
R = np.eye(3) + np.dot(sin(angle),axis_skewed) + (1-cos(angle))*np.dot(axis_skewed,axis_skewed); | ||
v1n= np.dot(v1n,R) | ||
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v2n= np.cross(vnorm,v1n); # v2 is a vector in the same plane but perpendicular to v1n | ||
v2n= v2n/np.linalg.norm(v2n) | ||
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v1n= np.dot(v1n,np.linalg.inv(cell)) # back to fractional | ||
v2n= np.dot(v2n,np.linalg.inv(cell)) # back to fractional | ||
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grid= np.zeros((npx*npy,3)) | ||
ip= 0 | ||
for ix in np.linspace(-1.5,1.5,npx): | ||
for iy in np.linspace(-1.5,1.5,npy): | ||
grid[ip]= (v1n*ix + v2n*iy + p1)*[nx,ny,nz] | ||
ip= ip + 1 | ||
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grid_x, grid_y, grid_z= grid[:,0], grid[:,1], grid[:,2] | ||
plane= ndimage.map_coordinates(CHGCAR.chg[0],[grid_x, grid_y, grid_z], mode="wrap") | ||
px,py=np.mgrid[-1.5:1.5:npx+0j,-1.5:1.5:npy+0j] | ||
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plt.rcParams["figure.figsize"]=[ 8,8] | ||
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plt.plot([0],[0],'ko',ms=9 ) | ||
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plt.plot( np.dot(np.dot(v1,cell),np.dot(v1n,cell)) , np.dot(np.dot(v1,cell),np.dot(v2n,cell)) , 'ko',ms=9 ) | ||
#plt.text( np.dot(np.dot(v1,cell),np.dot(v1n,cell)) , np.dot(np.dot(v1,cell),np.dot(v2n,cell))-0.1 , 'p1', alpha= 0.2) | ||
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plt.plot( np.dot(np.dot(v2,cell),np.dot(v1n,cell)) , np.dot(np.dot(v2,cell),np.dot(v2n,cell)) , 'ko',ms=9 ) | ||
#plt.text( np.dot(np.dot(v2,cell),np.dot(v1n,cell)) , np.dot(np.dot(v2,cell),np.dot(v2n,cell))-0.1 , 'p2', alpha= 0.2) | ||
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#CIM1= plt.imshow(plane.reshape(npx,npy).T, origin='lower', extent=(-1.5, 1.5, -1.5, 1.5), alpha=0.4, cmap='spectral') | ||
CIM1= plt.imshow(plane.reshape(npx,npy).T, origin='lower', extent=(-1.5, 1.5, -1.5, 1.5), alpha=1, vmin=-.2,vmax=.2, cmap='bwr') | ||
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#plt.contour(px,py,plane.reshape(npx,npy)) | ||
CL1= plt.contour(px,py,plane.reshape(npx,npy),np.arange(0.05,10,0.02), colors=["black"]) | ||
CL2= plt.contour(px,py,plane.reshape(npx,npy),[0], colors=["red"]) | ||
CL3= plt.contour(px,py,plane.reshape(npx,npy),np.arange(-0.05,-10,-0.02), colors=["blue"]) | ||
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plt.grid(True) | ||
plt.tick_params(size=10,width=1.5,pad=20, labelsize=22) | ||
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plt.savefig("CHGCAR.ps") | ||
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plt.ion() | ||
plt.show() | ||
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