Stoichiometry controlled conversion efficiency in nanostructured heterojunction solar cell of CdS/CuInS sub(X)Se sub(2-X) grown by chemical ion exchange method at room temperature
Here in the present paper, we report on growth of stoichiometric and nonstoichiometric nanostructured heterojunction solar cell of CdS/CuInS sub(X)Se sub(2-X) varying X from 0 to 2 in the interval of 0.5 using cost effective, simple, chemical ion exchange method at room temperature on ITO glass subs...
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Veröffentlicht in: | Solar energy 2011-07, Vol.85 (7), p.1316-1321 |
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Sprache: | eng |
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Zusammenfassung: | Here in the present paper, we report on growth of stoichiometric and nonstoichiometric nanostructured heterojunction solar cell of CdS/CuInS sub(X)Se sub(2-X) varying X from 0 to 2 in the interval of 0.5 using cost effective, simple, chemical ion exchange method at room temperature on ITO glass substrate. The as-grown varying composition solar cells annealed at 200 [deg]C in air and characterized for structural, compositional, optical and illumination studies. The X-ray diffraction pattern obtained from CdS/CuInS sub(X)Se sub(2-X) solar cell confirms the formation of CuInSe sub(2), CuInS sub(0.5)Se sub(1.5), CuInS sub(1)Se sub(1), CuInS sub(1.5)Se sub(0.5) and CuInS sub(2) phases having tetragonal structure with varying crystallite size from 19, 19.37, 28, 33 and 20 nm respectively. The energy dispersive X-ray analysis (EDAX) confirms the expected elemental composition in the heterojunction solar cell. Optical absorbance analysis confirms composition controlled electronic transitions in the thin films while energy band gap observed to be red shifted with increase the value of X. The solar energy conversion efficiency achieved upon illuminating to 100 mW/cm[super]2 observed to be 0.27%, 0.06%, 0.17%, 0.02% and 0.23% for CuInSe sub(2), CuInS sub(0.5)Se sub(1.5), CuInS sub(1)Se sub(1), CuInS sub(1.5)Se sub(0.5) and CuInS sub(2) respectively, which correspond for stoichiometric dependent electron-hole pair generation and separation phenomenon. |
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ISSN: | 0038-092X |
DOI: | 10.1016/j.solener.2011.03.013 |