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通过重取代掺杂改善CsInAgCl的光学和热电性能:基于密度泛函理论的见解

Improving the optical and thermoelectric properties of CsInAgCl with heavy substitutional doping: a DFT insight.

作者信息

Bhamu K C, Haque Enamul, Praveen C S, Kumar Nandha, Yumnam G, Hossain Md Anwar, Sharma Gautam

机构信息

PMC Division, CSIR-National Chemical Laboratory Pune 411008 Maharashtra India

Department of Physics, Gramin Mahila P. G. College Sikar 332024 Rajasthan India.

出版信息

RSC Adv. 2021 Jan 29;11(10):5521-5528. doi: 10.1039/d0ra01840f. eCollection 2021 Jan 28.

Abstract

The next-generation indium-based lead-free halide material CsInAgCl 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 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 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 K) for the n-type carrier after Pb-doping, which is ∼3.5 times higher than in the pristine case (0.6 mW m K) at 500 K.

摘要

下一代基于铟的无铅卤化物材料CsInAgCl因其良好的空气稳定性和无毒特性,在光伏应用方面具有潜力。然而,其宽带隙(>3 eV)不适合太阳光谱,因此降低了其在器件应用中的光电效率。在此,我们通过第一性原理研究报告了通过替代掺杂实现的从2.85 eV到0.65 eV的显著带隙降低及其对光电和光热发电特性的影响。结果预测,Sn/Pb以及Ga和Cu共掺杂将显著提高价带最大值(VBM)附近的态密度,从而降低带隙并使VBM向上移动,而碱金属(K/Rb)会略微增加带隙。在共掺杂情况下,在肖克利 - 奎塞尔极限附近观察到一个强吸收峰,而在Sn/Pb掺杂情况下,我们在太阳光谱可见光区域的中部注意到一个峰值。Cu - Ga/Pb/Sn掺杂时带隙性质为间接带隙,在Ga - Cu共掺杂情况下观察到带隙从2.85 eV显著降低到0.65 eV。我们观察到Pb掺杂后n型载流子的功率因子(PF)显著增加(2.03 mW m K),在500 K时比原始情况(0.6 mW m K)高约3.5倍。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4f74/8694724/03ac602c2bba/d0ra01840f-f2.jpg

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