2015
DOI: 10.1149/2.0171503jss
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Structural Evolution of Multilayer SnS/Cu/ZnS Stack to Phase-Pure Cu2ZnSnS4Thin Films by Thermal Processing

Abstract: In this work, thin films of phase-pure Cu 2 ZnSnS 4 (CZTS) were developed from a stack of binary metal sulfides by post-deposition thermal processing. The precursor stack SnS/Cu/ZnS was grown by sequential electrodeposition of SnS and Cu layers followed by thermal evaporation of ZnS layer. The transformation from binary/ternary composition to phase-pure CZTS was studied using different experimental tools such as X-ray diffraction (XRD), Raman spectroscopy, scanning electron microscopy (SEM), transmission elect… Show more

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Cited by 26 publications
(14 citation statements)
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“…2d). The observed Sn 3d 5/2 peak centered at 486.3 eV and the spin-orbit splitting of 8.5 eV are typical for Sn(IV) 24,43,47,61,6769,73 . This assignment is supported by an analysis of the Sn M 4,5 N 4,5 N 4,5 Auger electron energy spectrum (Fig.…”
Section: Resultsmentioning
confidence: 83%
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“…2d). The observed Sn 3d 5/2 peak centered at 486.3 eV and the spin-orbit splitting of 8.5 eV are typical for Sn(IV) 24,43,47,61,6769,73 . This assignment is supported by an analysis of the Sn M 4,5 N 4,5 N 4,5 Auger electron energy spectrum (Fig.…”
Section: Resultsmentioning
confidence: 83%
“…This broadening is a result of an additional relaxation path for the L 2 (2p 1/2 ) hole due to L 2 L 3 M 4,5 Coster-Cronig transition, which reduces the lifetime of the hole and broadens the Cu2p 1/2 peak 71 . The positions of peaks, the distance between them (19.9 eV), the absence of an additional contribution at around 934/954 eV, as well as the absence of paramagnetic Cu(II) satellite peaks at ~940–945 eV 72 indicate that copper is present in the sample solely as Cu(I) typically found in CZTS NCs 24,43,47,61,6769,73 . Nevertheless, as the differences reported in the literature between the positions of Cu(I) and Cu(II) compounds (oxides and chalcogenides) are rather small, we examined additionally with high-resolution XPS spectra the range of the Auger electron peak of copper, which is more sensitive to the chemical surrounding than the XPS peaks.…”
Section: Resultsmentioning
confidence: 93%
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“…Figure a presents the Cu 2p core level spectra which exhibits binding energies for the Cu 2p 3/2 and Cu 2p 1/2 peaks at ranges between 931.8–932.3 and 952–951.1 eV, respectively. There is also a peak splitting of 19.8 eV, indicating the formation of Cu(I) . Furthermore, the satellite peak of Cu 2p 3/2 which is characteristic of Cu 2+ is not present, indicating the absence of any Cu 2+ compound .…”
Section: Resultsmentioning
confidence: 78%
“…The possibility could be ternary phase such as Cu 2 Sn 3 S 7 and Cu 3 SnS 4 or binary phases such as SnS 2 . The presence of Cu 2 Sn 3 S 7 and Cu 3 SnS 4 phases was ruled out, because no peaks at 375 cm -1 and 268 cm -1 , 348 cm -1 and 295 cm -1 were observed, respectively[18][19]. Hence, SnS 2 was the main second phase in the referenced CTS.…”
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confidence: 99%