Skip to content

Commit 42fd50b

Browse files
authored
Merge pull request #1 from JunkeJiang/pero
Release perov-1-0
2 parents e8c8e53 + 0e5455a commit 42fd50b

Some content is hidden

Large Commits have some content hidden by default. Use the searchbox below for content that may be hidden.

41 files changed

+30915
-0
lines changed

CHANGELOG.md

+5
Original file line numberDiff line numberDiff line change
@@ -0,0 +1,5 @@
1+
# Changelog
2+
3+
## perov-1-0
4+
5+
First public release under CC-BY-SA license

README

+97
Original file line numberDiff line numberDiff line change
@@ -0,0 +1,97 @@
1+
============================================
2+
Parametrization for metal halide perovskites
3+
============================================
4+
5+
(c) 2017, Marcus Elstner, Karlsruher Institut für Technologie
6+
[original mio set]
7+
8+
(c) 2024, Junke Jiang, INSA Rennes
9+
[extension with I, Cs, Pb, recalculating all tables for consistency]
10+
11+
All rights reserved
12+
13+
This work is licensed under the Creative Commons Attribution-ShareAlike 4.0
14+
International License. To view a copy of this license, consult the LICENSE file
15+
or visit http://creativecommons.org/licenses/by-sa/4.0/ .
16+
17+
NOTE: The rights holder(s) for this work explicitly require that the attribution
18+
conditions of this license are enforced. Use in part or in whole of this data is
19+
permitted only under the condition that the scientific background of the
20+
Licensed Material will be CITED IN ANY PUBLICATIONS ARISING FROM ITS USE. The
21+
required references are specified in this file and must be included in resulting
22+
works.
23+
24+
25+
General information
26+
===================
27+
28+
This set was designed to describe the electronic structure of 2D and 3D metal
29+
halide perovskites. The parameters of H, C, and N may slightly deviate from mio-1-1.
30+
We refer to the detailed documentation in the Slater-Koster files for further
31+
information. The compression radii of Cs have been taken from Ref.[JCTC13], the
32+
power of the confinement potential, however, is slightly different.
33+
34+
Note: This set assumes that you use shell-resolved SCC in DFTB. In case you use
35+
the DFTB+ code, you can achieve it by setting `OrbitalResolvedSCC = Yes`.
36+
37+
38+
Maximal angular momenta
39+
-----------------------
40+
H: s
41+
C: p
42+
N: p
43+
I: p
44+
Cs: s
45+
Pb: p
46+
47+
48+
Spin constants
49+
--------------
50+
51+
Note, the calculation of the spin constants follows here for all elements the
52+
convention as used for the Hubbard U values: For non-occupied atomic orbitals
53+
(orbitals above HOMO), the corresponding value of the HOMO is used.
54+
55+
H:
56+
-0.07174
57+
C:
58+
-0.03062 -0.02505
59+
-0.02505 -0.02265
60+
N:
61+
-0.03318 -0.02755
62+
-0.02755 -0.02545
63+
Cs:
64+
-0.00949
65+
I:
66+
-0.01445 -0.01132
67+
-0.01132 -0.01145
68+
Pb:
69+
-0.01335 -0.00932
70+
-0.00932 -0.01097
71+
72+
73+
Repulsive energy:
74+
========================================
75+
76+
NOTABENE: NO REPULSIVE potential is provided; there is a dummy spline only.
77+
The SKFs CANNOT be used to do structural relaxation.
78+
79+
80+
Relevant publications
81+
=====================
82+
83+
[PRMat25] J. Jiang et al., Phys. Rev. Materials 9, 023803 (2025).
84+
85+
[JCTC13] M. Wahiduzzaman et al., J. Chem. Theory Comput. 9, 9, 4006 (2013).
86+
87+
[PRB98] M. Elstner, D. Porezag, G. Jungnickel, J. Elsner, M. Haugk,
88+
Th. Frauenheim, S. Suhai, and G. Seifert, Phys. Rev. B 58, 7260 (1998).
89+
90+
91+
Required references
92+
===================
93+
94+
H,C,N - H,C,N: [PRMat25,PRB98]
95+
H,C,N,I,Cs,Pb - I: [PRMat25]
96+
H,C,N,I,Cs,Pb - Cs: [PRMat25,JCTC13]
97+
H,C,N,I,Cs,Pb - Pb: [PRMat25]

0 commit comments

Comments
 (0)