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Breathing bands due to molecular order in CH3NH3PbI3
•The electronic gaps of MAPbI3 change largely depending on the molecular orientation.•This change appears at several levels of approximation.•It is due to the interactions between the inorganic and organic moieties.•This effect may be important for optical performance. CH3NH3PbI3 perovskite is nowad...
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Published in: | Computational materials science 2018-02, Vol.142, p.361-371 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | •The electronic gaps of MAPbI3 change largely depending on the molecular orientation.•This change appears at several levels of approximation.•It is due to the interactions between the inorganic and organic moieties.•This effect may be important for optical performance.
CH3NH3PbI3 perovskite is nowadays amongst the most promising photovoltaic materials for energy conversion. We have studied by ab initio calculations, using several levels of approximation – namely density functional theory including spin-orbit coupling and quasi-particle corrections by means of the GW method, as well as pseudopotential self-interaction corrections, the role of the methylammonium orientation on the electronic structure of this perovskite. We have considered many molecular arrangements within 2×2×2 supercells, showing that the relative orientation of the organic molecules is responsible for a huge band gap variation up to 2 eV. The band gap sizes are related to distortions of the PbI3 cage, which are in turn due to electrostatic interactions between this inorganic frame and the molecules. The strong dependence of the band gap on the mutual molecular orientation is confirmed at all levels of approximations. Our results suggest then that the coupling between the molecular motion and the interactions of the molecules with the inorganic cage could help to explain the widening of the absorption spectrum of CH3NH3PbI3 perovskite, consistent with the observed white spectrum. |
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ISSN: | 0927-0256 1879-0801 |
DOI: | 10.1016/j.commatsci.2017.10.039 |