Issue 44, 2025

Formamidinium-based Pb–Sn mixed-halide perovskite solar cells with near-optimal bandgap: FAPb1−xSnx(I0.8Br0.2)3

Abstract

The development of lead–tin (Pb–Sn) binary perovskites with ideal bandgaps (1.3–1.4 eV) is crucial for single-junction perovskite solar cells (PSCs) to approach the Shockley–Queisser efficiency limit. Compositional engineering, the most effective strategy for improving PSC efficiency, offers a promising route to tune the perovskite bandgap into the ideal range. In this study, we developed FA-based Pb–Sn mixed-halide perovskites, FAPb1−xSnx(I0.8Br0.2)3, via compositional engineering to target near-optimal bandgaps (∼1.4 eV), improve crystallinity and enhance absorption coefficient. Structural and morphological analyses reveal that Sn incorporation stabilizes the photoactive phase of pure FA-based perovskites, whereas Pb incorporation promotes the formation of dense films. This synergistic effect enables Pb–Sn binary PSCs to outperform their Pb-only and Sn-only counterparts. Furthermore, it is found that a Sn content of x = 0.4 yields optimal photovoltaic performance under ambient conditions and the lowest photovoltage deficit. Our analysis of the charge recombination processes indicates that structural disorder and band alignment act as competing factors governing the photovoltage deficit. This study elucidates how compositional engineering fine-tunes the optoelectronic properties of perovskites and provides insights into developing novel Pb–Sn binary PSCs with near-optimal bandgaps.

Graphical abstract: Formamidinium-based Pb–Sn mixed-halide perovskite solar cells with near-optimal bandgap: FAPb1−xSnx(I0.8Br0.2)3

Supplementary files

Article information

Article type
Paper
Submitted
01 Jul 2025
Accepted
08 Oct 2025
First published
31 Oct 2025

Nanoscale, 2025,17, 25859-25867

Formamidinium-based Pb–Sn mixed-halide perovskite solar cells with near-optimal bandgap: FAPb1−xSnx(I0.8Br0.2)3

Y. Chen, Y. F. Tay, M. Li, T. Z. Oo, S. Y. Chiam, Y. M. Lam, T. C. Sum and L. H. Wong, Nanoscale, 2025, 17, 25859 DOI: 10.1039/D5NR02776D

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