Tail state formation in solar cell materials: First principles analyses of zincblende, chalcopyrite, kesterite and hybrid perovskite crystals
Mitsutoshi Nishiwaki, Keisuke Nagaya, Masato Kato, Shohei Fujimoto,, Hitoshi Tampo, Tetsuhiko Miyadera, Masayuki Chikamatsu, Hajime Shibata, and, Hiroyuki Fujiwara

TL;DR
This study uses first-principles calculations to analyze tail state formation in various solar cell materials, revealing that cation disordering significantly contributes to tail states in some compounds, while hybrid perovskites show minimal tailing.
Contribution
Developed a general theoretical scheme comparing experimental Urbach energies with DFT-derived absorption edges to analyze tail state formation in solar cell materials.
Findings
Tail states are negligible in CdTe, CISe, CGSe, and hybrid perovskites.
Large Urbach energies in CZTSe and CZTS are due to cation disordering.
Hybrid perovskite CH3NH3PbI3 shows sharp absorption edges consistent with minimal tail states.
Abstract
Tail state formation in solar cell absorbers leads to a detrimental effect on solar cell performance. Nevertheless, the characterization of the band tailing in experimental semiconductor crystals is generally difficult. In this article, to determine the tail state generation in various solar cell materials, we have developed a quite general theoretical scheme in which the experimental Urbach energy is compared with the absorption edge energy derived from density functional theory (DFT) calculation. For this purpose, the absorption spectra of solar cell materials, including CdTe, CuInSe2 (CISe), CuGaSe2 (CGSe), Cu2ZnSnSe4 (CZTSe), Cu2ZnSnS4 (CZTS) and hybrid perovskites, have been calculated by DFT particularly using very-high-density k meshes. As a result, we find that the tail state formation is negligible in CdTe, CISe, CGSe and hybrid perovskite polycrystals. However, coevaporated…
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