2009
DOI: 10.1016/j.tsf.2008.11.024
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Radiative recombination in Cu2ZnSnSe4 monograins studied by photoluminescence spectroscopy

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Cited by 158 publications
(131 citation statements)
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“…1(d), the modes at 169, 173 cm -1 , 196.6 and 234 cm -1 , as reported earlier [6] and assigned to CZTSe, can be seen. The Cu x Se mode at 261 cm -1 can also be found at a few small spots randomly distributed across the surface.…”
supporting
confidence: 77%
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“…1(d), the modes at 169, 173 cm -1 , 196.6 and 234 cm -1 , as reported earlier [6] and assigned to CZTSe, can be seen. The Cu x Se mode at 261 cm -1 can also be found at a few small spots randomly distributed across the surface.…”
supporting
confidence: 77%
“…However, the usefulness of such methods depends critically on the availability of high quality material, with sharp and resolved features in the optical spectra. Despite the high record efficiency the structural quality currently achieved in Cu 2 ZnSn(S,Se) 4 is rather low: in the majority of publications the photoluminescence (PL) spectra reveal only one broad, low intensity band ascribed to radiative recombination of free electrons and holes localised at shallow acceptors [6]. The width of this band and its asymmetric shape suggest the influence of band tails induced by randomly distributed high concentrations of charged defects.…”
mentioning
confidence: 99%
“…[9][10][11][12] The absorption coefficient is a > 10 4 cm À1 at photon energies >1.05 eV, and Urbach energy is E Ur % 170 meV. The calculated curve fits the measured spectrum well in the range <1.4 eV.…”
mentioning
confidence: 53%
“…So far, experimental results are reported only for the first absorption edge around 1 eV. [9][10][11][12] In this manuscript, we report on our findings on the absorption behavior of CZTSe absorber films above this photon energy and present experimental results which confirm the existence of a lone conduction band.…”
mentioning
confidence: 60%
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