1993
DOI: 10.1006/jssc.1993.1242
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Anion Distributions and Phase Transitions in CuS1-xSex(x = 0-1) Studied by Raman Spectroscopy

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Cited by 259 publications
(172 citation statements)
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“…Since these phases are formed from the surface of the layer they absorb the signal from the underlying IGS to a large extent. Raman spectroscopy measurements of samples annealed at 250°C reveal a slight blue shift in the position of the Cu-Se peak, consistent with the formation of CuSe from Cu-rich selenides [17]. Due to the volume increase accompanying the formation of CuSe, no signal can be detected from the IGS layer in this spectrum.…”
Section: Resultssupporting
confidence: 64%
“…Since these phases are formed from the surface of the layer they absorb the signal from the underlying IGS to a large extent. Raman spectroscopy measurements of samples annealed at 250°C reveal a slight blue shift in the position of the Cu-Se peak, consistent with the formation of CuSe from Cu-rich selenides [17]. Due to the volume increase accompanying the formation of CuSe, no signal can be detected from the IGS layer in this spectrum.…”
Section: Resultssupporting
confidence: 64%
“…When the selenization was interrupted at 250°C, no indium selenide peaks were observed in the Raman spectrum, however two new peaks were present at 263 and 275cm -1 . The peak at 263cm -1 has been associated with CuSe [25], however no reports of an accompanying peak at 275cm -1 could be found in the literature. The diffractogram measured from a sample with similarly interrupted selenization (displayed in Figure 1) indicates the presence of both CuSe and In 2 Se 3 phases, therefore the absence of the indium selenide peaks in the Raman spectrum is attributed to a phase separation through the depth of the layer, leading to the Raman signal being generated solely within the copper selenide surface layer.…”
Section: Resultsmentioning
confidence: 98%
“…The peak at 240 cm −1 is attributed to the presence of trigonal elementary selenium ͑Se͒, 13 while the peak at 261 cm −1 is characteristic of Cu-Se compounds. The absence of intense low-frequency bands at 17 and 42 cm −1 characteristic of the covellite-type structure ͑CuSe͒, 14 and the analysis of the XRD spectra, points to a different binary, probably Cu 2 Se, though the coexistence of the covellite CuSe phase cannot be discarded. Figure 3 ͑left͒ shows an OM image of the surface of the as-grown sample.…”
Section: ͑1͒mentioning
confidence: 99%