2017
DOI: 10.1016/j.solmat.2017.04.022
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Influence of the copper content on the optical properties of CZTSe thin films

Abstract: We present an optical spectroscopy study of Cu 2 ZnSnSe 4 (CZTSe) thin films deposited on Mo/glass substrates. The [Cu]/[Zn+Sn] ratio in these films varies from nearly stoichiometric to strongly Cu deficient and Zn rich. Increasing Cu deficiency and Zn excess widens the bandgap E g , determined using photoluminescence excitation (PLE) at 4.2 K, from 0.99 eV to 1.03 eV and blue shifts the dominant band in the photoluminescence (PL) spectra from 0.83 eV to 0.95 eV. The PL spectra of the near stoichiometric film … Show more

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Cited by 35 publications
(34 citation statements)
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“…Conversely, LP devices have a higher J SC value (26.1 mA/cm 2 ) in comparison to that seen in HP devices (23.7 mA/cm 2 ). Similar observations were made by Yakushev et al for Cu 2 ZnSnSe 4 (CZTSe) devices with varying Cu/(Zn+Sn) and Zn/Sn ratios and were attributed to the degree of Cu-Zn order/disorder in the crystal lattice (Yakushev et al, 2017). EQE plots for LP and HP devices are shown in Fig.…”
Section: Also the Ionised V Cusupporting
confidence: 85%
See 1 more Smart Citation
“…Conversely, LP devices have a higher J SC value (26.1 mA/cm 2 ) in comparison to that seen in HP devices (23.7 mA/cm 2 ). Similar observations were made by Yakushev et al for Cu 2 ZnSnSe 4 (CZTSe) devices with varying Cu/(Zn+Sn) and Zn/Sn ratios and were attributed to the degree of Cu-Zn order/disorder in the crystal lattice (Yakushev et al, 2017). EQE plots for LP and HP devices are shown in Fig.…”
Section: Also the Ionised V Cusupporting
confidence: 85%
“…revealed comparable temperature trends in PL spectra of CZTSe thin lms with varying Cu content (Yakushev et al, 2017).…”
Section: Resultsmentioning
confidence: 68%
“…As in the film the P2 band quenches by 70 K. At temperatures above 200 K the solar cell spectra show a broad band at 0.9 eV. Such bands, observed earlier in CZTS [28] and CZTSe [20,23,24], were attributed to band-to-band (BB) transitions, involving the recombination of free electrons from the conduction band with free holes from the valence band. The P3 band in the PL spectra of the solar cell gradually quenches with raising temperature however it retains a relatively high intensity up to temperatures of 300 K. High concentrations of charged defects generate tails in the density of states (DOS) of the conduction and valence bands of semiconductors.…”
Section: Resultsmentioning
confidence: 80%
“…The rate of this shift (j-shift) is 14 meV per decade of laser power change for the CZTSe/Mo film and decreases to 13 meV/decade for the cell spectra as shown in Table 1. The characteristic asymmetric shape of the P1 band, the invariance of this shape on the excitation intensity and the significant j-shifts suggest that the radiative recombination mechanism of this band is associated with band tails generated by spatial potential fluctuations due to high concentrations of charged defects [18,20,[23][24][25][26][27]. The P3 band in the PL spectra of the cell also increases its intensity at higher excitation.…”
Section: Resultsmentioning
confidence: 96%
“…However, this tendency is opposite to those found in Cu2ZnSnSe4, where the band gap increases with copper deficiency. 38 On the other hand, the Cu-Zn lattice disorder in CZTS can induce a change in the band gap of about 0.2 eV. 39 According to this concept, an increase of the band gap is related to an increase of degree of ordering in the samples.…”
mentioning
confidence: 99%