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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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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
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author Brivio, Federico
Caetano, Clovis
Walsh, Aron
author_facet Brivio, Federico
Caetano, Clovis
Walsh, Aron
author_sort Brivio, Federico
collection PubMed
description [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.
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spelling pubmed-50423582016-10-03 Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy Brivio, Federico Caetano, Clovis Walsh, Aron J Phys Chem Lett [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. American Chemical Society 2016-03-07 2016-03-17 /pmc/articles/PMC5042358/ /pubmed/26952337 http://dx.doi.org/10.1021/acs.jpclett.6b00226 Text en Copyright © 2016 American Chemical Society This is an open access article published under a Creative Commons Attribution (CC-BY) License (http://pubs.acs.org/page/policy/authorchoice_ccby_termsofuse.html) , which permits unrestricted use, distribution and reproduction in any medium, provided the author and source are cited.
spellingShingle Brivio, Federico
Caetano, Clovis
Walsh, Aron
Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title_full Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title_fullStr Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title_full_unstemmed Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title_short Thermodynamic Origin of Photoinstability in the CH(3)NH(3)Pb(I(1–x)Br(x))(3) Hybrid Halide Perovskite Alloy
title_sort thermodynamic origin of photoinstability in the ch(3)nh(3)pb(i(1–x)br(x))(3) hybrid halide perovskite alloy
url 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
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