Pseudohalide-Induced Moisture Tolerance in Perovskite CH3NH3Pb(SCN)2I Thin Films

Two pseudohalide thiocyanate ions (SCN−) have been used to replace two iodides in CH3NH3PbI3, and the resulting perovskite material was used as the active material in solar cells. In accelerated stability tests, the CH3NH3Pb(SCN)2I perovskite films were shown to be superior to the conventional CH3NH...

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Published inAngewandte Chemie International Edition Vol. 54; no. 26; pp. 7617 - 7620
Main Authors Jiang, Qinglong, Rebollar, Dominic, Gong, Jue, Piacentino, Elettra L., Zheng, Chong, Xu, Tao
Format Journal Article
LanguageEnglish
Published Weinheim WILEY-VCH Verlag 22.06.2015
WILEY‐VCH Verlag
Wiley Subscription Services, Inc
EditionInternational ed. in English
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Summary:Two pseudohalide thiocyanate ions (SCN−) have been used to replace two iodides in CH3NH3PbI3, and the resulting perovskite material was used as the active material in solar cells. In accelerated stability tests, the CH3NH3Pb(SCN)2I perovskite films were shown to be superior to the conventional CH3NH3PbI3 films as no significant degradation was observed after the film had been exposed to air with a relative humidity of 95 % for over four hours, whereas CH3NH3PbI3 films degraded in less than 1.5 hours. Solar cells based on CH3NH3Pb(SCN)2I thin films exhibited an efficiency of 8.3 %, which is comparable to that of CH3NH3PbI3 based cells fabricated in the same way. The replacement of two iodides by two pseudohalide thiocyanate ions in CH3NH3PbI3 results in a perovskite material with superior tolerance to moisture when used as the active material of a solar cell. For the CH3NH3Pb(SCN)2I perovskite films, no significant degradation was observed after the film had been exposed to air with a relative humidity of 95 % for over four hours, whereas the CH3NH3PbI3 films degraded in less than 1.5 hours.
Bibliography:ark:/67375/WNG-NR80BS47-D
Financial support from the U.S. NSF (CBET-1150617) is gratefully acknowledged.
NSF - No. CBET-1150617
ArticleID:ANIE201503038
istex:AA7EC1641D833482E95439ECED86BAF7A59C1295
Financial support from the U.S. NSF (CBET‐1150617) is gratefully acknowledged.
ISSN:1433-7851
1521-3773
DOI:10.1002/anie.201503038