## Abstract Optical absorption spectra of CuIn~5~Se~8~ and CuGa~3~Se~5~ single crystals have been investigated. The energy gap __E__ ~g~ for CuIn~5~Se~8~ (CuGa~3~Se~5~) was found to be varied from 1.27 (1.79) to 1.21 (1.71) eV in the temperature range between 10 and 300 K. The temperature dependenc
Urbach's tail in the absorption spectra of CuIn5Se8and CuGa3Se5single crystals
✍ Scribed by Arushanov, E. ;Levcenko, S. ;Syrbu, N. N. ;Nateprov, A. ;Tezlevan, V. ;Merino, J. M. ;León, M.
- Publisher
- John Wiley and Sons
- Year
- 2006
- Tongue
- English
- Weight
- 147 KB
- Volume
- 203
- Category
- Article
- ISSN
- 0031-8965
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✦ Synopsis
Abstract
Optical absorption spectra of CuIn~5~Se~8~ and CuGa~3~Se~5~ single crystals grown by chemical vapour transport were investigated in the range of 10–300 K. The logarithmic variation of the absorption coefficient with photon energy observed in both compounds just below the fundamental absorption edge shows a linear dependence at different temperatures in agreement with Urbach's rule. The Urbach energy as well as the energy associated with the electron/exciton–phonon interaction related to Urbach's tail are estimated. The latter is found to be around 52 (41) meV for CuIn~5~Se~8~ (CuGa~3~Se~5~). It is lower than that {58 (60) meV} earlier reported for these compounds and confirms higher structural quality of samples studied. It is shown that the temperature of the Urbach energy can be modeled in CuIn~5~Se~8~ (CuGa~3~Se~5~) as an Einstein oscillator with the Einstein temperature equal to 222 (266) K. It is found that in the material studied structural disorder is dominant at 300 K. It may be caused by some compositional deviation from stoichiometry. The latter was observed in the studied samples by using the EDAX method. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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## Abstract The ellipsometric spectra of CuIn~3~Se~5~, CuGa~3~Se~5~ and CuGa~5~Se~8~ ordered vacancy compounds (OVC) have been studied in the spectral range from 0.8 to 4.4 eV. The structures observed in the measured spectra were analyzed by fitting the second derivative of the experimental spectru