2016
DOI: 10.1016/j.solmat.2015.10.004
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Systematic compositional changes and their influence on lattice and optoelectronic properties of Cu2ZnSnSe4 kesterite solar cells

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Cited by 61 publications
(50 citation statements)
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“…Sample after the selenization process of 410 °C for 60 min is a solid mixture of cubic increased with an increase in the [Zn]/[Sn] molar ratio in the metal precursors. Similar results can be observed in the Cu-based I-II-IV-VI semiconductors [27,28] . However, only XRD patterns of samples may not confirmed the real phases of samples.…”
Section: Resultssupporting
confidence: 86%
See 1 more Smart Citation
“…Sample after the selenization process of 410 °C for 60 min is a solid mixture of cubic increased with an increase in the [Zn]/[Sn] molar ratio in the metal precursors. Similar results can be observed in the Cu-based I-II-IV-VI semiconductors [27,28] . However, only XRD patterns of samples may not confirmed the real phases of samples.…”
Section: Resultssupporting
confidence: 86%
“…The Raman shifts of samples at around 181 cm −1 are closed to that for ternary shift to high frequency. Similar results can also be observed in the Cu-based I-II-IV-VI and Cu-based I-III-VI semiconductors [28,30] . We can conclude that the band in Raman shift at around 181 cm −1 belongs to the kesterite AZTSe phase and is influenced with the Zn content in the samples.…”
Section: Resultssupporting
confidence: 84%
“…The kesterite composition correlates with the measured bandgap and Cu-poor kesterite exhibits a higher bandgap than Cu-rich kesterite. [30,31] Utilizing the bandgap measurements from Figure 3d we deduce that the kesterite composition is less Cu-poor for Na compared to K for the same nominal Sn content. Conclusively, the remnant Sn not incorporated into the kesterite phase leads to the appearance of Sn(S,Se) 2 secondary phase.…”
Section: Resultsmentioning
confidence: 89%
“…The results of the analysis are reflected at the top of the CMZTSSe thin films because the effective analysis depth of Raman spectra with 514 nm excitation is about 108 nm . Besides, the Cu content will be decreased when the Raman intensity of CZTSe at about 170 cm −1 decreases . Therefore, the Cu 2 Mn 0.05 Zn 0.95 Sn(S,Se) 4 absorber surface is more Cu‐poor compared with the pure‐CZTSSe.…”
Section: Resultsmentioning
confidence: 99%