Intrinsic Instability of the Hybrid Halide Perovskite Semiconductor CH3NH3PbI3

Yue Yu Zhang, Shiyou Chen, Peng Xu, Hongjun Xiang, Xin Gao Gong, Aron Walsh, Su Huai Wei

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104 Citations (Scopus)

Abstract

The organic-inorganic hybrid perovskite CH3NH3PbI3 has attracted significant interest for its high performance in converting solar light into electrical power with an efficiency exceeding 20%. Unfortunately, chemical stability is one major challenge in the development of CH3NH3PbI3 solar cells. It was commonly assumed that moisture or oxygen in the environment causes the poor stability of hybrid halide perovskites, however, here we show from the first-principles calculations that the room-temperature tetragonal phase of CH3NH3PbI3 is thermodynamically unstable with respect to the phase separation into CH3NH3I+PbI2, i.e., the disproportionation is exothermic, independent of the humidity or oxygen in the atmosphere. When the structure is distorted to the low-temperature orthorhombic phase, the energetic cost of separation increases, but remains small. Contributions from vibrational and configurational entropy at room temperature have been considered, but the instability of CH3NH3PbI3 is unchanged. When I is replaced by Br or Cl, Pb by Sn, or the organic cation CH3NH3 by inorganic Cs, the perovskites become more stable and do not phase-separate spontaneously. Our study highlights that the poor chemical stability is intrinsic to CH3NH3PbI3 and suggests that element-substitution may solve the chemical stability problem in hybrid halide perovskite solar cells.

Original languageEnglish
Article number036104
JournalChinese Physics Letters
Volume35
Issue number3
DOIs
Publication statusPublished - 2018 Mar

Bibliographical note

Funding Information:
The work at Fudan University was supported by the Special Funds for Major State Basic Research, National Natural Science Foundation of China (NSFC), and Project of Shanghai Municipality (16520721600). S.C. was supported by NSFC under Grant No 91233121, Shanghai Rising-Star Program (14QA1401500) and CC of ECNU. The work at Bath was supported by the Royal Society, the ERC and EPSRC under Grant Nos EP/M009580/1 and EP/K016288/1. S.H.W. was supported by the National Key Research and Development Program of China under Grant No 2016YFB0700700, and the National Natural Science Foundation of China under Grant Nos 51672023, 11634003 and U1530401. **Corresponding author. Email: chensy@ee.ecnu.edu.cn; xggong@fudan.edu.cn ○c 2018 Chinese Physical Society and IOP Publishing Ltd

Publisher Copyright:
© 2018 Chinese Physical Society and IOP Publishing Ltd.

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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