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Discovery of two new Cu–Sn chalco–halides for potential solar absorber applications

Abstract:
We explore multiple-cation chalco–halide phase fields evaluated by their synthetic accessibility using machine learning models. Exploratory synthesis guided by computational tools leads to the discovery of two new compounds; CuSn2SI3 and Cu0.35Sn5.29S2I7, their structures, and electronic and optical properties are reported herein. This is the first report of a stable quaternary compound in the Cu–Sn–S–I phase field. The two new compounds show related crystal structures where Sn4S2I4 layers are a common structural motif in both. These Sn4S2I4 layers are connected by Cu2I2 layers and disordered Cu–Sn–I layers, forming the three-dimensional structures of CuSn2SI3 and Cu0.35Sn5.29S2I7 respectively. Electronic band structure calculations using density functional theory show the presence of a direct band gap in CuSn2SI3 and suggest anisotropic transport, in line with the layered structure of the compound. A mixture of the two compounds with ∼86% CuSn2SI3, shows a band gap in the visible region, close to 2.1 eV and a significant photo-induced charge carrier mobility of ∼1.3 cm2 V−1 s−1. This demonstrates Cu–Sn chalco–halides can form a promising phase space to explore for solar absorber materials, with further design and tuning of band gap.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1039/d5ta06204g

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author
ORCID:
0000-0003-3943-5389
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author
ORCID:
0000-0001-8697-5412



Publisher:
Royal Society of Chemistry
Journal:
Journal of Materials Chemistry A More from this journal
Volume:
14
Issue:
27
Pages:
17257–17271
Publication date:
2026-03-20
Acceptance date:
2026-03-14
DOI:
EISSN:
2050-7496
ISSN:
2050-7488


Language:
English
Keywords:
Source identifiers:
3899587
Deposit date:
2026-03-30
ARK identifier:

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