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Structural and optical properties of the Cu2ZnSnSe4 thin films grown by nano-ink coating and selenization
Authors:Ying Liu  De-Yi Kong  Hui You  Chi-lai Chen  Xin-hua Lin  Jürgen Brugger
Affiliation:1. State Key Laboratory of Transducer Technology, Institute of Intelligent Machines, Chinese Academy of Sciences, No. 350 Shushan Road, Hefei, Anhui Province, 230031, P.R. China
2. Department of Chemistry, University of Science and Technology of China, No. 96, Jin Zhai Road Baohe District, Hefei, Anhui Province, 230026, P.R. China
3. Microsystems Laboratory, école Polytechnique Fédérale de Lausanne (EPFL), EPFL-STI-IMT-LMIS1, Station 17, CH-1015, Lausanne, Switzerland
Abstract:Quaternary semiconductor Cu2ZnSnSe4 (CZTSe) is a very promising alternative to semiconductors based on indium (In) and gallium (Ga) as solar absorber material due to its direct band gap, inherent high absorption coefficient (>104 cm?1) and abundance of cheap elements zinc (Zn) and tin (Sn). In this study, high quality CZTSe thin films were successfully synthesized by a green and low-cost solution based non-vacuum method, which involves spin coating non-toxic solvent-based CZTSe nano-inks onto Mo coated soda lime glass substrates followed by selenization with elemental Se vapor. The effect of selenization temperature on structural, morphological, compositional and optical properties of CZTSe films are investigated using X-ray diffraction (XRD), Raman spectroscopy, scanning electron microscopy (SEM), energy dispersive spectroscopy (EDS) and photoluminescence spectroscopy. XRD and Raman analysis indicates that a tetragonal stannite-type structured CZTSe is formed. Depend on the selenization temperature, the dense and compact films with grain sizes from 200 nm (500 °C) up to about 1 μm (580 °C) are obtained. EDS measurement indicates that the composition ratios of the prepared CZTSe films are copper-poor and zinc-rich nature. The CZTSe films are p-type conductivity confirmed by a hot point probe method. Photoluminescence spectrum shows slightly asymmetric narrow bands with a maximum of intensity at 0.92 eV. The dependence of the photoluminescence on the excitation temperature reveals a decrease in the intensity of the photoluminescence bands. An absorption coefficient exceeding 104 cm?1 and the band gap energy about 0.87 eV of the studied films are determined by an absorption spectroscopy.
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