2016
DOI: 10.1016/j.jallcom.2015.09.186
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XRD studies of an electrochemically co-deposited Cu–Zn–Sn precursor and formation of a Cu2ZnSnSe4 absorber for thin-film solar cells

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Cited by 29 publications
(10 citation statements)
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“…The peaks at 78/80 cm −1 can be attributed to E (TO/LO) symmetries of CZTSe 37,42 . Similar Raman peaks were obtained by Dimitrievska et al, 42 Juskenas et al, 38 and Khare et al 37 In addition, two weak peaks on the right shoulders of the peaks at 232 and 236 cm −1 were referred to the MoSe 2 phase. Consequently, the analysis of the Raman data suggested that the selenization of the precursor films led to the formation of CZTSe and CZTSSe with quasi‐ordered kesterite structure and the films contained both the KS and ST phases.…”
Section: Resultssupporting
confidence: 81%
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“…The peaks at 78/80 cm −1 can be attributed to E (TO/LO) symmetries of CZTSe 37,42 . Similar Raman peaks were obtained by Dimitrievska et al, 42 Juskenas et al, 38 and Khare et al 37 In addition, two weak peaks on the right shoulders of the peaks at 232 and 236 cm −1 were referred to the MoSe 2 phase. Consequently, the analysis of the Raman data suggested that the selenization of the precursor films led to the formation of CZTSe and CZTSSe with quasi‐ordered kesterite structure and the films contained both the KS and ST phases.…”
Section: Resultssupporting
confidence: 81%
“…The peak at 172 cm −1 can be referred to the mode A2 of ST (175.40 сm −1 ) composed of the vibration of Se anions 37‐39 . The obtained peaks at 232 cm −1 (sample A1) and 236 сm −1 (sample A2) correspond to the vibrations of symmetry Е (TO/LO) of KS (233.02 сm −1 ) generated by the anion and cation vibrations of Cu 2 ZnSnSe 4.…”
Section: Resultsmentioning
confidence: 95%
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“…A similar asymmetrically broadening dominant Raman peak of the CZTSe was observed in few works (Khare et al, 2012;Djemour et al, 2013;Juskenas et al, 2016;Rey et al, 2014;Schelhas et al, 2017). For…”
Section: Raman Spectroscopysupporting
confidence: 80%
“…Two stage process found to be preferable and very successful for growth of Cu 2 ZnSnSe 4 films [4] due to its scalability with large throughput. In first step, metallic stacks of Cu-Zn-Sn were deposited onto glass/Mo coated glass substrate using several techniques such as co-evaporation [5], sputtering [6][7][8][9][10][11][12], vacuum evaporation [13], electro deposition [14][15][16], e-beam evaporation [17], spin coating [18] and knife edge coating [19]. Later, selenization of metallic precursors was carried out using elemental selenium/H 2 Se gas in presence of inert Ar/N 2 atmosphere at elevated temperature (≥450 °C).…”
Section: Introductionmentioning
confidence: 99%