Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer

A star-shaped polymer enables inverted perovskite solar cells with efficiency over 22% and a very high fill factor of 0.862. Stabilizing high-efficiency perovskite solar cells (PSCs) at operating conditions remains an unresolved issue hampering its large-scale commercial deployment. Here, we report...

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Published inScience advances Vol. 7; no. 28
Main Authors Cao, Qi, Li, Yongjiang, Zhang, Hong, Yang, Jiabao, Han, Jian, Xu, Ting, Wang, Shuangjie, Wang, Zishuai, Gao, Bingyu, Zhao, Junsong, Li, Xiaoqiang, Ma, Xiaoyan, Zakeeruddin, Shaik Mohammed, Sha, Wei E. I., Li, Xuanhua, Grätzel, Michael
Format Journal Article
LanguageEnglish
Published American Association for the Advancement of Science 01.07.2021
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Summary:A star-shaped polymer enables inverted perovskite solar cells with efficiency over 22% and a very high fill factor of 0.862. Stabilizing high-efficiency perovskite solar cells (PSCs) at operating conditions remains an unresolved issue hampering its large-scale commercial deployment. Here, we report a star-shaped polymer to improve charge transport and inhibit ion migration at the perovskite interface. The incorporation of multiple chemical anchor sites in the star-shaped polymer branches strongly controls the crystallization of perovskite film with lower trap density and higher carrier mobility and thus inhibits the nonradiative recombination and reduces the charge-transport loss. Consequently, the modified inverted PSCs show an optimal power conversion efficiency of 22.1% and a very high fill factor (FF) of 0.862, corresponding to 95.4% of the Shockley-Queisser limited FF (0.904) of PSCs with a 1.59-eV bandgap. The modified devices exhibit excellent long-term operational and thermal stability at the maximum power point for 1000 hours at 45°C under continuous one-sun illumination without any significant loss of efficiency.
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These authors contribute equally to this work.
ISSN:2375-2548
2375-2548
DOI:10.1126/sciadv.abg0633