Abstract
The next-generation indium-based lead-free halide material Cs2InAgCl6is 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 eVviasubstitutional 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 bandgapviashifting 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−1K−2) for the n-type carrier after Pb-doping, which is ∼3.5 times higher than in the pristine case (0.6 mW m−1K−2) at 500 K.
Original language | English |
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Pages (from-to) | 5521-5528 |
Number of pages | 8 |
Journal | RSC Advances |
Volume | 11 |
Issue number | 10 |
DOIs | |
State | Published - Jan 29 2021 |
Externally published | Yes |
Funding
KCB and CSP acknowledge DST and DST-SERB for SERB-NPDF and INSPIRE Faculty fellowships with award numbers IFA-18 PH217 and PDF/2017/002876, respectively. The research used resources at the National Energy Research Scientic Computing Center (NERSC), which is supported by the Office of Science of the USDOE, United States, under contract no. DE-AC02-05CH11231. The high-performance computational facility of the Centre for Development of Advanced Computing, Pune, was also used for the present investigation.
Funders | Funder number |
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DST-SERB | |
SERB-NPDF | IFA-18 PH217 |
U.S. Department of Energy | DE-AC02-05CH11231 |
Office of Science | |
Department of Science and Technology, Ministry of Science and Technology, India |