Abstract
Thin films of p-type Cu3BiS3 with an orthorhombic wittichenite structure, a semiconductor with high potential for thin film solar cell absorber layers, were synthesised by thermal annealing of Cu and Bi precursors, magnetron sputtered on Mo/glass substrate, with a layer of thermo-evaporated S. The elemental composition, structural and electronic properties are studied. The Raman spectrum shows four modes with the dominant peak at 292 cm−1. Photoreflectance spectra demonstrate two band gaps EgX and EgY, associated with the X and Y valence sub-bands, and their evolution with temperature. Fitting the temperature dependencies of the band-gaps gives values of 1.24 and 1.53 eV for EgX and EgY at 0 K as well as the average phonon energy. Photoluminescence spectra at 5 K reveal two bright and broad emission bands at 0.84 and 0.99 eV, which quench with an activation energy of 40 meV. The photocurrent excitation measurements demonstrate a photoresponse and suggest a direct allowed nature of the band gap.
Original language | English |
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Pages (from-to) | 195-199 |
Journal | Thin Solid Films |
Volume | 562 |
Early online date | 26 Apr 2014 |
DOIs | |
Publication status | Published - 1 Jul 2014 |
Keywords
- Thin films
- Solar cells
- Semiconductors
- Electronic structure
- Raman spectroscopy
- Photoreflectance
- Photoluminescence
- CU-SB
- SEMICONDUCTORS
- CHALCOPYRITE
- DEPENDENCE
- AGINS2
- BANDS