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Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer
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...
Autores principales: | , , , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
American Association for the Advancement of Science
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8262814/ https://www.ncbi.nlm.nih.gov/pubmed/34233877 http://dx.doi.org/10.1126/sciadv.abg0633 |
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author | 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 |
author_facet | 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 |
author_sort | Cao, Qi |
collection | PubMed |
description | 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. |
format | Online Article Text |
id | pubmed-8262814 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | American Association for the Advancement of Science |
record_format | MEDLINE/PubMed |
spelling | pubmed-82628142021-07-16 Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer 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 Sci Adv Research Articles 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. American Association for the Advancement of Science 2021-07-07 /pmc/articles/PMC8262814/ /pubmed/34233877 http://dx.doi.org/10.1126/sciadv.abg0633 Text en Copyright © 2021 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). https://creativecommons.org/licenses/by-nc/4.0/This is an open-access article distributed under the terms of the Creative Commons Attribution-NonCommercial license (https://creativecommons.org/licenses/by-nc/4.0/) , which permits use, distribution, and reproduction in any medium, so long as the resultant use is not for commercial advantage and provided the original work is properly cited. |
spellingShingle | Research Articles 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 Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title | Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title_full | Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title_fullStr | Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title_full_unstemmed | Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title_short | Efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
title_sort | efficient and stable inverted perovskite solar cells with very high fill factors via incorporation of star-shaped polymer |
topic | Research Articles |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8262814/ https://www.ncbi.nlm.nih.gov/pubmed/34233877 http://dx.doi.org/10.1126/sciadv.abg0633 |
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