2014
DOI: 10.1016/j.materresbull.2013.10.009
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The investigation of CuxZnSnSe4 bulks with x=1.4–2.2 for debating the Cu excess and Cu deficiency used in thin-film solar cells

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Cited by 23 publications
(14 citation statements)
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“…As can be seen, all the samples show strong Raman peaks at 172 cm -1 , 196 cm -1 and 233 cm -1 respectively, which are in good agreement with the Raman scattering feature of CZTSe reported in the literature[26,30]. The intense peak at 196 cm -1 corresponds to the main vibrational A 1 symmetry modes from CZTSe[31].…”
supporting
confidence: 87%
“…As can be seen, all the samples show strong Raman peaks at 172 cm -1 , 196 cm -1 and 233 cm -1 respectively, which are in good agreement with the Raman scattering feature of CZTSe reported in the literature[26,30]. The intense peak at 196 cm -1 corresponds to the main vibrational A 1 symmetry modes from CZTSe[31].…”
supporting
confidence: 87%
“…The open circles in Figure 7.13 show the hole Hall mobilities plotted versus hole concentration (p) obtained from Cu-deficient/Cu-rich CZTSe thin films by Kuo and Tsega [62]. All these data fall within the stoichiometric μ h versus p plot region.…”
Section: Effect Of Stoichiometrymentioning
confidence: 88%
“…These measurements were performed on Cu-deficient CZTS [43], Cu-deficient CZTSe [59], Cu-deficient and Zn-rich CZTSe [60], Cu-rich CZTSe [61], Cu-deficient/Cu-rich CZTSe [62], Cu-deficient and Sn-rich CZTSe [63], and Cudeficient CZTSSe [64]. These measurements were performed on Cu-deficient CZTS [43], Cu-deficient CZTSe [59], Cu-deficient and Zn-rich CZTSe [60], Cu-rich CZTSe [61], Cu-deficient/Cu-rich CZTSe [62], Cu-deficient and Sn-rich CZTSe [63], and Cudeficient CZTSSe [64].…”
Section: Effect Of Stoichiometrymentioning
confidence: 99%
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