A computational screen of Rb2BX6 perovskites (B=Si,Ge,Sn,Pt; X=Cl,Br,I) finds a 0.56 to 6.12 eV bandgap range and identifies Rb2SnI6 as the most promising solar absorber.
First-principles prediction into robust high-performance photovoltaic double perovskites A$_{2}$SiI$_{6}$ (A = K, Rb, Cs)
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abstract
Despite the exceeding 23\% photovoltaic efficiency achieved in organic-inorganic hybrid perovskite solar cells obtaining, the stable materials with desirable band gap are rare and are highly desired. With the aid of first-principles calculations, we predict a new promising family of nontoxic inorganic double perovskites (DPs), namely, silicon (Si)-based halides A$_{2}$SiI$_{6}$ (A = K, Rb, Cs; X = Cl, Br, I). This family containing the earth-abundant Si could be applied for perovskite solar cells (PSCs). Particularly A$_{2}$SiI$_{6}$ exhibits superb physical traits, including suitable band gaps of 0.84-1.15 eV, dispersive lower conduction bands, small carrier effective masses, wide photon absorption in the visible range. Importantly, the good stability at high temperature renders them as promising optical absorbers for solar cells.
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Unveiling the Optoelectronic Potential of Vacancy-Ordered Double Perovskites: A Computational Deep Dive
A computational screen of Rb2BX6 perovskites (B=Si,Ge,Sn,Pt; X=Cl,Br,I) finds a 0.56 to 6.12 eV bandgap range and identifies Rb2SnI6 as the most promising solar absorber.