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Potential efficiency improvement of CuSb(S1-x,Sex)2 thin film solar cells by the Zn(O,S) buffer layer optimization

•The CuSb(S,Se)2 solar cells with a structure of contact/CuSb(S,Se)2/buffer layer/i-nO/ZnO:Al/contact was studied.•CuSbS2 solar cell based on an experimental device (ɳ=3.2%) has been modeled.•Conventional CdS buffer layer replaced by Zn(O,S) buffer layers.•The influence of Se/(Se + S) ratio in the C...

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Bibliographic Details
Published in:Solar energy 2021-09, Vol.225, p.875-881
Main Authors: Saadat, M., Amiri, O., Mahmood, Peshawa H.
Format: Article
Language:English
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Summary:•The CuSb(S,Se)2 solar cells with a structure of contact/CuSb(S,Se)2/buffer layer/i-nO/ZnO:Al/contact was studied.•CuSbS2 solar cell based on an experimental device (ɳ=3.2%) has been modeled.•Conventional CdS buffer layer replaced by Zn(O,S) buffer layers.•The influence of Se/(Se + S) ratio in the CuSb(S1-x,Sex)2 absorber layer and oxygen content in the buffer layer on the performance of the solar cell was investigated.•The influence of carrier concentration of both CuSb(S1-x,Sex)2 absorber and buffer layers was investigated. An initial structure was designed based on CuSbS2 experimental data. Afterward, an investigation on the performance of contact/CuSb(S1-x,Sex)2 alloy/buffer layer/i-ZnO/ZnO:Al/contact has been carried out. The conventional CdS layer was replaced by Zn(O1-y,Sy) layer, and the influence of Se/(Se + S) ratio in the CuSb(S1-x,Sex)2 absorber layer and oxygen content in the buffer layer on the performance of the solar cell were investigated. The influence of carrier concentration of both CuSb(S1-x,Sex)2 absorber and buffer layers are studied to enhance the output performance of CuSb(S1-x,Sex)2 thin-film solar cells. After optimizing the Se content in the absorber layer and oxygen content in the buffer layer, the best device is delivered 5.85% efficiency. However, after optimization of donor concentration in buffer layer the conversion efficiency is further increased to 7.19% for CuSbS2 absorber and donor concentration of 1019 cm−3.
ISSN:0038-092X
1471-1257
DOI:10.1016/j.solener.2021.08.013