Over 12% efficient kesterite solar cell via back interface engineering

The effects of WO3 intermediate layer on the microstructure, electrical and defects properties of CZTSSe films are revealed for the first time, and high quality CZTSSe crystal and low back interface contact barrier are obtained. [Display omitted] Kesterite Cu2ZnSn(S,Se)4 (CZTSSe) has attracted consi...

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Veröffentlicht in:Journal of energy chemistry 2022-12, Vol.75, p.321-329
Hauptverfasser: Zhao, Yunhai, Yu, Zixuan, Hu, Juguang, Zheng, Zhuanghao, Ma, Hongli, Sun, Kaiwen, Hao, Xiaojing, Liang, Guangxing, Fan, Ping, Zhang, Xianghua, Su, Zhenghua
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container_end_page 329
container_issue
container_start_page 321
container_title Journal of energy chemistry
container_volume 75
creator Zhao, Yunhai
Yu, Zixuan
Hu, Juguang
Zheng, Zhuanghao
Ma, Hongli
Sun, Kaiwen
Hao, Xiaojing
Liang, Guangxing
Fan, Ping
Zhang, Xianghua
Su, Zhenghua
description The effects of WO3 intermediate layer on the microstructure, electrical and defects properties of CZTSSe films are revealed for the first time, and high quality CZTSSe crystal and low back interface contact barrier are obtained. [Display omitted] Kesterite Cu2ZnSn(S,Se)4 (CZTSSe) has attracted considerable attention as a non-toxic and earth-abundant solar cell material. During selenization of CZTSSe film at high temperature, the reaction between CZTSSe and Mo is one of the main reasons that result in unfavorable absorber and interface quality, which leads to large open circuit voltage deficit (VOC-def) and low fill factor (FF). Herein, a WO3 intermediate layer introduced at the back interface can effectually inhibit the unfavorable interface reaction between absorber and back electrode in the preliminary selenization progress; thus high-quality crystals are obtained. Through this back interface engineering, the traditional problems of phase segregation, voids in the absorber and over thick Mo(S,Se)2 at the back interface can be well solved, which greatly lessens the recombination in the bulk and at the interface. The increased minority carrier diffusion length, decreased barrier height at back interface contact and reduced deep acceptor defects give rise to systematic improvement in VOC and FF, finally a 12.66% conversion efficiency for CZTSSe solar cell has been achieved. This work provides a simple way to fabricate highly efficient solar cells and promotes a deeper understanding of the function of intermediate layer at back interface in kesterite-based solar cells.
doi_str_mv 10.1016/j.jechem.2022.08.031
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[Display omitted] Kesterite Cu2ZnSn(S,Se)4 (CZTSSe) has attracted considerable attention as a non-toxic and earth-abundant solar cell material. During selenization of CZTSSe film at high temperature, the reaction between CZTSSe and Mo is one of the main reasons that result in unfavorable absorber and interface quality, which leads to large open circuit voltage deficit (VOC-def) and low fill factor (FF). Herein, a WO3 intermediate layer introduced at the back interface can effectually inhibit the unfavorable interface reaction between absorber and back electrode in the preliminary selenization progress; thus high-quality crystals are obtained. Through this back interface engineering, the traditional problems of phase segregation, voids in the absorber and over thick Mo(S,Se)2 at the back interface can be well solved, which greatly lessens the recombination in the bulk and at the interface. 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[Display omitted] Kesterite Cu2ZnSn(S,Se)4 (CZTSSe) has attracted considerable attention as a non-toxic and earth-abundant solar cell material. During selenization of CZTSSe film at high temperature, the reaction between CZTSSe and Mo is one of the main reasons that result in unfavorable absorber and interface quality, which leads to large open circuit voltage deficit (VOC-def) and low fill factor (FF). Herein, a WO3 intermediate layer introduced at the back interface can effectually inhibit the unfavorable interface reaction between absorber and back electrode in the preliminary selenization progress; thus high-quality crystals are obtained. Through this back interface engineering, the traditional problems of phase segregation, voids in the absorber and over thick Mo(S,Se)2 at the back interface can be well solved, which greatly lessens the recombination in the bulk and at the interface. 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subjects Chemical Sciences
Crystal growth
Cu2ZnSn(S,Se)4
Interface contact quality
Material chemistry
Minority carrier diffusion length
WO3 intermediate layer
title Over 12% efficient kesterite solar cell via back interface engineering
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