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Improving the optical and thermoelectric properties of Cs2InAgCl6 with heavy substitutional doping: a DFT insight.
Bhamu, K C; Haque, Enamul; Praveen, C S; Kumar, Nandha; Yumnam, G; Hossain, Md Anwar; Sharma, Gautam.
Afiliação
  • Bhamu KC; PMC Division, CSIR-National Chemical Laboratory Pune 411008 Maharashtra India kcbhamu85@gmail.com.
  • Haque E; Department of Physics, Gramin Mahila P. G. College Sikar 332024 Rajasthan India.
  • Praveen CS; Department of Physics, Mawlana Bhashani Science and Technology University Santosh Tangail-1902 Bangladesh enamul.phy15@yahoo.com.
  • Kumar N; International School of Photonics, Cochin University of Science and Technology University Road, South Kalamassery, Kalamassery Ernakulam Kerala 682022 India.
  • Yumnam G; Inter University Centre for Nano Materials and Devices, Cochin University of Science and Technology University Road, South Kalamassery, Kalamassery Ernakulam Kerala 682022 India.
  • Hossain MA; The Abdus Salam International Centre for Theoretical Physics Strada Costiera 11 34151 Trieste Italy.
  • Sharma G; Department of Physics and Astronomy, University of Missouri Columbia 65211 USA.
RSC Adv ; 11(10): 5521-5528, 2021 Jan 28.
Article em En | MEDLINE | ID: mdl-35423116
ABSTRACT
The next-generation indium-based lead-free halide material Cs2InAgCl6 is promising for photovoltaic applications due to its good air stability and non-toxic behavior. However, its wide bandgap (>3 eV) is not suitable for the solar spectrum and hence reduces its photoelectronic efficiency for device applications. Here we report a significant bandgap reduction from 2.85 eV to 0.65 eV via substitutional doping and its effects on the optoelectronic and opto-thermoelectric properties from a first-principles study. The results predict that Sn/Pb and Ga and Cu co-doping will enhance the density of states significantly near the valence band maximum (VBM) and thus reduce the bandgap via shifting the VBM upward, while alkali metals (K/Rb) slightly increase the bandgap. A strong absorption peak near the Shockley-Queisser limit is observed in the co-doped case, while in the Sn/Pb-doped case, we notice a peak in the middle of the visible region of the solar spectrum. The nature of the bandgap is indirect with Cu-Ga/Pb/Sn doping, and a significant reduction in the bandgap, from 2.85 eV to 0.65 eV, is observed in the case of Ga-Cu co-doping. We observe a significant increase in the power factor (PF) (2.03 mW m-1 K-2) for the n-type carrier after Pb-doping, which is ∼3.5 times higher than in the pristine case (0.6 mW m -1 K-2) at 500 K.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2021 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2021 Tipo de documento: Article