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 Vol. 127; no. 26; pp. 7727 - 7730
Main Authors Jiang, Qinglong, Rebollar, Dominic, Gong, Jue, Piacentino, Elettra L., Zheng, Chong, Xu, Tao
Format Journal Article
LanguageEnglish
German
Published Weinheim WILEY-VCH Verlag 22.06.2015
WILEY‐VCH Verlag
Wiley Subscription Services, Inc
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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. Der Austausch von zwei Iodiden durch zwei Thiocyanat‐Pseudohalogenidionen in CH3NH3PbI3 resultiert in einem Perowskit mit verbesserter Feuchtigkeitstoleranz, wenn dieses als aktives Material einer Solarzelle verwendet wird. Die CH3NH3Pb(SCN)2I‐Perowskitfilme hatten sich nach vier Stunden in Luft mit einer relativen Feuchtigkeit von 95 % kaum zersetzt, während die CH3NH3PbI3‐Filme sich bereits innerhalb von weniger als anderthalb Stunden zersetzten.
Bibliography:Financial support from the U.S. NSF (CBET-1150617) is gratefully acknowledged.
ark:/67375/WNG-JF2PMBNR-Z
NSF - No. CBET-1150617
istex:148BC9459B7EA75F52DF6D98DCBA702E89F6D0D0
ArticleID:ANGE201503038
Financial support from the U.S. NSF (CBET‐1150617) is gratefully acknowledged.
ISSN:0044-8249
1521-3757
DOI:10.1002/ange.201503038