Theoretical insight into the CdS/FAPbI3 heterostructure: a promising visible-light absorber

Metal halide perovskites have drawn considerable attention thanks to their excellent optoelectronic performances. However, further development has been severely hampered by their poor stability. Recently, it has been confirmed experimentally that the optical performance of perovskites is significantly improved by the incorporation of a CdS layer. Based on this, first-principles calculations are conducted to probe the inherent mechanism, including the electronic structure, absorption spectra, strain effect, etc. The optimized geometric structure shows that the distance between the CdS layer and the FAPbI(3) layer is smaller than 3.0 angstrom, which implies that the CdS/FAPbI(3) heterostructure is more stable than common van der Waals heterostructures. Moreover, it is revealed that the electronic states at the band gap edge are from different component layers. It is further unveiled by Bader charge analysis that the electronic charge is transferred from the FAPbI(3) layer to the CdS layer, which is consistent with the charge density difference (CDD). In addition, the absorption coefficient in the CdS/FAPbI(3) heterostructure is remarkably enhanced, compared with that of pure perovskite FAPbI(3). Furthermore, the strain effect on the bandgap of the CdS/FAPbI(3) is also explored. These results shed new light on understanding and designing new kinds of highly efficient perovskite-based photovoltaic materials.

Automated summary

The optical performance of metal halide perovskites can be significantly improved by incorporating a CdS layer, which also enhances the stability of the CdS/FAPbI(3) heterostructure compared to common van der Waals heterostructures. Electronic states at the band gap edge come from different component layers, with electronic charge transferred from the FAPbI(3) layer to the CdS layer. Additionally, the absorption coefficient in the CdS/FAPbI(3) heterostructure is remarkably enhanced compared with pure perovskite FAPbI(3).