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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
in
Cell size
/ Copper
/ Copper zinc tin selenide
/ Crystallization
/ Diffraction patterns
/ Electrodeposition
/ Electron microscopes
/ Fabrication
/ Grain size
/ Partial pressure
/ Photovoltaic cells
/ Preferred orientation
/ Scanning electron microscopy
/ Selenide
/ Selenium
/ Solar cells
/ Substrates
/ Thin films
/ Tin
/ Tin selenide
/ X-ray diffraction
/ Zinc
2014
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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
by
in
Cell size
/ Copper
/ Copper zinc tin selenide
/ Crystallization
/ Diffraction patterns
/ Electrodeposition
/ Electron microscopes
/ Fabrication
/ Grain size
/ Partial pressure
/ Photovoltaic cells
/ Preferred orientation
/ Scanning electron microscopy
/ Selenide
/ Selenium
/ Solar cells
/ Substrates
/ Thin films
/ Tin
/ Tin selenide
/ X-ray diffraction
/ Zinc
2014
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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
in
Cell size
/ Copper
/ Copper zinc tin selenide
/ Crystallization
/ Diffraction patterns
/ Electrodeposition
/ Electron microscopes
/ Fabrication
/ Grain size
/ Partial pressure
/ Photovoltaic cells
/ Preferred orientation
/ Scanning electron microscopy
/ Selenide
/ Selenium
/ Solar cells
/ Substrates
/ Thin films
/ Tin
/ Tin selenide
/ X-ray diffraction
/ Zinc
2014
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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
Journal Article
CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure
2014
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Overview
Cu2ZnSnSe4 (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 (SnSex) 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.
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