2014
DOI: 10.1186/1556-276x-9-678
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CZTSe solar cells prepared by electrodeposition of Cu/Sn/Zn stack layer followed by selenization at low Se pressure

Abstract: 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 suppr… Show more

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Cited by 25 publications
(19 citation statements)
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“…The typical deposition time was about 15 seconds. Samples of the metallic precursors (4 cm 2 × 4 cm 2 in area) were reactively annealed in a laboratory-made furnace capable of working in vacuum (1 × 10 −4 Pa) or an inert gas (Ar) atmosphere [13]. The sample temperature, Sn temperature and the Se temperature are controlled individually.…”
Section: Methodsmentioning
confidence: 99%
See 1 more Smart Citation
“…The typical deposition time was about 15 seconds. Samples of the metallic precursors (4 cm 2 × 4 cm 2 in area) were reactively annealed in a laboratory-made furnace capable of working in vacuum (1 × 10 −4 Pa) or an inert gas (Ar) atmosphere [13]. The sample temperature, Sn temperature and the Se temperature are controlled individually.…”
Section: Methodsmentioning
confidence: 99%
“…Their values are still far from the record cell efficiency of above 21% for Cu(In,Ga)Se 2 [4] and CdTe [5]. Because of the thermodynamic stability of CZTS(e) thin films [6] and the volatility of tin selenide (SnSe x ) [7], a two-step process was generally used to prepare CZTSe thin films [2,3,[7][8][9][10][11][12][13]. A precursor with all or part of the CZTS(e) components was prepared first by either a vacuum or non-vacuum method and was then treated by subsequent thermal annealing to improve the crystallinity.…”
Section: Introductionmentioning
confidence: 99%
“…The Gibbs free energy changes of the two reactions are negative, implying that both of the chemical reactions may occur spontaneously. However, in our previous study [22], the formation of MoSe 2 layer is very slow when the selenization of metal precursor is at a low Se partial pressure atmosphere. Therefore, we can conclude that the formation of the MoSe 2 layer in sample A3 is dominated by the reaction of 2SnSe 2 + Mo = 2SnSe + MoSe 2 , owing to the excess of SnSe x from the reactions of Cu x Sn y + 2Se x (g) → Cu 2− x Se + SnSe x during selenization.…”
Section: Resultsmentioning
confidence: 99%
“…Samples of the metallic precursors were reactively selenized in a laboratory-made furnace (not a tubular furnace) capable of working in vacuum (10 −4 Pa) or an inert gas (Ar) atmosphere [22]. The sample temperature, Sn temperature and the Se temperature are controlled individually.…”
Section: Methodsmentioning
confidence: 99%
“…Recently, various approaches have been developed to fabricate the absorber layers, briefly including vacuumbased deposition and non-vacuum-based solution process; both strategies have yielded a remarkable improvement in photovoltaic performance [2][3][4][5][6][7][8]. Compared to vacuumbased approaches, non-vacuum technologies such as electrodeposition approach [9][10][11], milling dispersion approach [12], nanoparticle-based approach [13][14][15][16], hydrazine-based approach [17][18][19], and sol-gel approach [20][21][22][23][24] are more feasible for industrial production. Among those solution-based process, the hydrazine-based deposition has made the great progress, achieving the power conversion efficiency (PCE) of 12.6 % [25].…”
Section: Introductionmentioning
confidence: 99%