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Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy

[Image: see text] The formation of solid-solutions of iodide, bromide, and chloride provides the means to control the structure, band gap, and stability of hybrid halide perovskite semiconductors for photovoltaic applications. We report a computational investigation of the CH(3)NH(3)PbI(3)/CH(3)NH(3...

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Detalles Bibliográficos
Autores principales: Brivio, Federico, Caetano, Clovis, Walsh, Aron
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2016
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5042358/
https://www.ncbi.nlm.nih.gov/pubmed/26952337
http://dx.doi.org/10.1021/acs.jpclett.6b00226
Descripción
Sumario:[Image: see text] The formation of solid-solutions of iodide, bromide, and chloride provides the means to control the structure, band gap, and stability of hybrid halide perovskite semiconductors for photovoltaic applications. We report a computational investigation of the CH(3)NH(3)PbI(3)/CH(3)NH(3)PbBr(3) alloy from density functional theory with a thermodynamic analysis performed within the generalized quasi-chemical approximation. We construct the phase diagram and identify a large miscibility gap, with a critical temperature of 343 K. The observed photoinstability in some mixed-halide solar cells is explained by the thermodynamics of alloy formation, where an initially homogeneous solution is subject to spinodal decomposition with I and Br-rich phases, which is further complicated by a wide metastable region defined by the binodal line.