Mohnish Pandey, Korina Kuhar, and Karsten W. Jacobsen
Phys. Chem. C, 2017, 121 (33), pp 17780–17786
Database contains chalcopyrite, kesterite, and wurtzite polymorphs of II–IV–V2 and III–III–V2 materials investigated for light absorption in the visible range. The data set includes stability information, band gaps, and carrier effective masses.
Mohnish Pandey, Korina Kuhar, and Karsten W. Jacobsen
Phys. Chem. C, 2017, 121 (33), pp 17780–17786
Download database: abx2.db
key |
description |
unit |
---|---|---|
|
E-hull |
eV |
|
Kohn Sham band gap |
eV |
|
Effective electron mass |
\(m_e\) |
|
Effective hole mass |
\(m_e\) |
|
Derivative discontinuity (GLLB-SC) |
eV |
|
Energy per atom |
eV |
|
Uncertanty of the convex hull energy |
eV |
|
Uncertanty of the total energy |
eV |
|
Direct band gap (GLLB-SC) |
eV |
|
Indirect band gap (GLLB-SC) |
eV |
|
Direct band gap (TB09) |
eV |
|
Indirect band gap (TB09) |
eV |
|
Crystal system |
|
|
Phase |
|
|
Short chemical formula |
|
|
Total energy (mBEEF) |
eV |
mBEEF energies and the corresponding uncertainties for three phases:
# creates: enthalpy.png
import numpy as np
import matplotlib.pyplot as plt
from ase.db import connect
db = connect('abx2.db')
names = sorted(row.short_name for row in db.select(phase='ST'))
x = np.arange(len(names))
plt.figure(figsize=(10, 5))
for phase, mark, color in zip(['KT', 'ST', 'CP'], 'osv', 'rbg'):
y = []
dy = []
for row in db.select(phase=phase, sort='short_name'):
y.append(row.E_relative_perAtom)
dy.append(row.E_uncertanty_perAtom)
print(x, y)
plt.errorbar(x, y, yerr=dy, color=color, fmt=mark, label=phase)
y = []
dy = []
for row in db.select(phase='ST', sort='short_name'):
y.append(row.E_hull)
dy.append(row.E_uncertanty_hull)
plt.errorbar(x, y, yerr=dy, color='k', fmt='x', label=r'$\Delta E$')
plt.xticks(x, names, rotation=70)
for xx in x:
plt.axvline(xx + 0.5, color='lightgrey')
plt.axhline(0, color='grey')
plt.xlim(-0.5, x[-1] + 0.5)
plt.legend()
plt.ylabel(r'$E$ [eV/atom]')
plt.savefig('enthalpy.png', bbox_inches='tight')