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https://hdl.handle.net/20.500.14094/90003865
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2025-08-10
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90003865 (fulltext)
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メタデータID
90003865
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open access
出版タイプ
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タイトル
Rotation mechanism of methylammonium molecules in organometal halide perovskite in cubic phase: An ab initio molecular dynamics study
著者
Shimamura, Kohei ; Hakamata, Tomoya ; Shimojo, Fuyuki ; Kalia, Rajiv K. ; Nakano, Aiichiro ; Vashishta, Priya
著者ID
A1705
研究者ID
1000060772647
KUID
https://kuid-rm-web.ofc.kobe-u.ac.jp/search/detail?systemId=35fc37f823944137520e17560c007669
著者名
Shimamura, Kohei
島村, 孝平
シマムラ, コウヘイ
所属機関名
システム情報学研究科
著者名
Hakamata, Tomoya
著者名
Shimojo, Fuyuki
著者名
Kalia, Rajiv K.
著者名
Nakano, Aiichiro
著者名
Vashishta, Priya
言語
English (英語)
収録物名
Journal of Chemical Physics
巻(号)
145(22)
ページ
224503-224503
出版者
AIP Publishing
刊行日
2016-12-14
公開日
2018-01-01
抄録
Rotation of methylammonium (CH(3)NH(3) or MA) molecules is believed to govern the excellent transport properties of photocarriers in the MA lead iodide (MAPbI(3)) perovskite. Of particular interest is its cubic phase, which exists in industrially important films at room temperature. In order to investigate the rotational behaviors of the MA molecules, we have performed ab initio molecular dynamics simulations of cubic-MAPbI(3) at room temperature. There are two types of rotational motions of MA molecules in a crystalline PbI(3) cage: reorientation of a whole molecule and intramolecular rotation around the C-N bond within MA molecules. Using a cubic symmetry-assisted analysis (CSAA), we found that the prominent orientation of the C-N bond is the crystalline < 110 > directions, rather than the < 100 > and < 111 > directions. Rapid rotation around the C-N bond is also observed, which easily occurs when the rotational axis is parallel to the < 110 > directions according to the CSAA. To explain the atomistic mechanisms underlying these CSAA results, we have focused on the relation between H-I hydrogen bonds and the orientation of an MA molecule. Here, the hydrogen bonds were defined by population analysis, and it has been found that, while H atoms in the CH(3) group (HC) hardly interacts with I atoms, those in the NH(3) group (HN) form at least one hydrogen bond with I atoms and their interatomic distances are in a wide range, 2.2-3.7 angstrom. Based on these findings, we have given a possible explanation to why the < 110 > directions are preferred. Namely, the atomic arrangement and interatomic distance between MA and surrounding I atoms are most suitable for the formation of hydrogen bonds. In addition to films, these results are potentially applicable to the rotational behaviors in bulk MAPbI(3) as well, considering that the atomistic structure and time constants regarding the rotation of MA molecules statistically agree with bulk experiments.
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システム情報学研究科
学術雑誌論文
権利
©2016 AIP Publishing. This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. The following article appeared in Journal of Chemical Physics 145(22), 224503 and may be found at http://dx.doi.org/10.1063/1.4971791
関連情報
DOI
https://doi.org/10.1063/1.4971791
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資源タイプ
journal article
ISSN
0021-9606
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eISSN
1089-7690
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