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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
Cu(2)ZnSnSe(4) (CZTSe) thin films are prepared by the electrodeposition of stack copper/tin/zinc (Cu/Sn/Zn) precursors, followed by selenization with a tin source at a substrate temperature of 530°C. Three selenization processes were performed herein to study the effects of the source of tin on the...
Autores principales: | , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer
2014
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4275120/ https://www.ncbi.nlm.nih.gov/pubmed/25593559 http://dx.doi.org/10.1186/1556-276X-9-678 |
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author | Yao, Liyong Ao, Jianping Jeng, Ming-Jer Bi, Jinlian Gao, Shoushuai He, Qing Zhou, Zhiqiang Sun, Guozhong Sun, Yun Chang, Liann-Be Chen, Jian-Wun |
author_facet | Yao, Liyong Ao, Jianping Jeng, Ming-Jer Bi, Jinlian Gao, Shoushuai He, Qing Zhou, Zhiqiang Sun, Guozhong Sun, Yun Chang, Liann-Be Chen, Jian-Wun |
author_sort | Yao, Liyong |
collection | PubMed |
description | Cu(2)ZnSnSe(4) (CZTSe) thin films are prepared by the electrodeposition of stack copper/tin/zinc (Cu/Sn/Zn) precursors, followed by selenization with a tin source at a substrate temperature of 530°C. Three selenization processes were performed herein to study the effects of the source of tin on the quality of CZTSe thin films that are formed at low Se pressure. Much elemental Sn is lost from CZTSe thin films during selenization without a source of tin. The loss of Sn from CZTSe thin films in selenization was suppressed herein using a tin source at 400°C (A2) or 530°C (A3). A copper-poor and zinc-rich CZTSe absorber layer with Cu/Sn, Zn/Sn, Cu/(Zn + Sn), and Zn/(Cu + Zn + Sn) with metallic element ratios of 1.86, 1.24, 0.83, and 0.3, respectively, was obtained in a selenization with a tin source at 530°C. The crystallized CZTSe thin film exhibited an increasingly (112)-preferred orientation at higher tin selenide (SnSe( x )) partial pressure. The lack of any obvious Mo-Se phase-related diffraction peaks in the X-ray diffraction (XRD) diffraction patterns may have arisen from the low Se pressure in the selenization processes. The scanning electron microscope (SEM) images reveal a compact surface morphology and a moderate grain size. CZTSe solar cells with an efficiency of 4.81% were produced by the low-cost fabrication process that is elucidated herein. |
format | Online Article Text |
id | pubmed-4275120 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2014 |
publisher | Springer |
record_format | MEDLINE/PubMed |
spelling | pubmed-42751202015-01-15 CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure Yao, Liyong Ao, Jianping Jeng, Ming-Jer Bi, Jinlian Gao, Shoushuai He, Qing Zhou, Zhiqiang Sun, Guozhong Sun, Yun Chang, Liann-Be Chen, Jian-Wun Nanoscale Res Lett Nano Express Cu(2)ZnSnSe(4) (CZTSe) thin films are prepared by the electrodeposition of stack copper/tin/zinc (Cu/Sn/Zn) precursors, followed by selenization with a tin source at a substrate temperature of 530°C. Three selenization processes were performed herein to study the effects of the source of tin on the quality of CZTSe thin films that are formed at low Se pressure. Much elemental Sn is lost from CZTSe thin films during selenization without a source of tin. The loss of Sn from CZTSe thin films in selenization was suppressed herein using a tin source at 400°C (A2) or 530°C (A3). A copper-poor and zinc-rich CZTSe absorber layer with Cu/Sn, Zn/Sn, Cu/(Zn + Sn), and Zn/(Cu + Zn + Sn) with metallic element ratios of 1.86, 1.24, 0.83, and 0.3, respectively, was obtained in a selenization with a tin source at 530°C. The crystallized CZTSe thin film exhibited an increasingly (112)-preferred orientation at higher tin selenide (SnSe( x )) partial pressure. The lack of any obvious Mo-Se phase-related diffraction peaks in the X-ray diffraction (XRD) diffraction patterns may have arisen from the low Se pressure in the selenization processes. The scanning electron microscope (SEM) images reveal a compact surface morphology and a moderate grain size. CZTSe solar cells with an efficiency of 4.81% were produced by the low-cost fabrication process that is elucidated herein. Springer 2014-12-15 /pmc/articles/PMC4275120/ /pubmed/25593559 http://dx.doi.org/10.1186/1556-276X-9-678 Text en Copyright © 2014 Yao et al.; licensee Springer. http://creativecommons.org/licenses/by/4.0 This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited. |
spellingShingle | Nano Express Yao, Liyong Ao, Jianping Jeng, Ming-Jer Bi, Jinlian Gao, Shoushuai He, Qing Zhou, Zhiqiang Sun, Guozhong Sun, Yun Chang, Liann-Be Chen, Jian-Wun CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title | CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title_full | CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title_fullStr | CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title_full_unstemmed | CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title_short | CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure |
title_sort | cztse solar cells prepared by electrodeposition of cu/sn/zn stack layer followed by selenization at low se pressure |
topic | Nano Express |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4275120/ https://www.ncbi.nlm.nih.gov/pubmed/25593559 http://dx.doi.org/10.1186/1556-276X-9-678 |
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