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Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)

[Image: see text] The two-dimensional (2D) mixed halide perovskite PEA(2)Pb(I(1–x)Br(x))(4) exhibits high phase stability under illumination as compared to the three-dimensional (3D) counterpart MAPb(I(1–x)Br(x))(3). We explain this difference using a thermodynamic theory that considers the sum of a...

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Autores principales: Chen, Zehua, Xue, Haibo, Brocks, Geert, Bobbert, Peter A., Tao, Shuxia
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2023
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9926482/
https://www.ncbi.nlm.nih.gov/pubmed/36816777
http://dx.doi.org/10.1021/acsenergylett.2c02463
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author Chen, Zehua
Xue, Haibo
Brocks, Geert
Bobbert, Peter A.
Tao, Shuxia
author_facet Chen, Zehua
Xue, Haibo
Brocks, Geert
Bobbert, Peter A.
Tao, Shuxia
author_sort Chen, Zehua
collection PubMed
description [Image: see text] The two-dimensional (2D) mixed halide perovskite PEA(2)Pb(I(1–x)Br(x))(4) exhibits high phase stability under illumination as compared to the three-dimensional (3D) counterpart MAPb(I(1–x)Br(x))(3). We explain this difference using a thermodynamic theory that considers the sum of a compositional and a photocarrier free energy. Ab initio calculations show that the improved compositional phase stability of the 2D perovskite is caused by a preferred I–Br distribution, leading to a much lower critical temperature for halide segregation in the dark than for the 3D perovskite. Moreover, a smaller increase of the band gap with Br concentration x and a markedly shorter photocarrier lifetime in the 2D perovskite reduce the driving force for phase segregation under illumination, enhancing the photostability.
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spelling pubmed-99264822023-02-15 Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4) Chen, Zehua Xue, Haibo Brocks, Geert Bobbert, Peter A. Tao, Shuxia ACS Energy Lett [Image: see text] The two-dimensional (2D) mixed halide perovskite PEA(2)Pb(I(1–x)Br(x))(4) exhibits high phase stability under illumination as compared to the three-dimensional (3D) counterpart MAPb(I(1–x)Br(x))(3). We explain this difference using a thermodynamic theory that considers the sum of a compositional and a photocarrier free energy. Ab initio calculations show that the improved compositional phase stability of the 2D perovskite is caused by a preferred I–Br distribution, leading to a much lower critical temperature for halide segregation in the dark than for the 3D perovskite. Moreover, a smaller increase of the band gap with Br concentration x and a markedly shorter photocarrier lifetime in the 2D perovskite reduce the driving force for phase segregation under illumination, enhancing the photostability. American Chemical Society 2023-01-13 /pmc/articles/PMC9926482/ /pubmed/36816777 http://dx.doi.org/10.1021/acsenergylett.2c02463 Text en © 2023 The Authors. Published by American Chemical Society https://creativecommons.org/licenses/by/4.0/Permits the broadest form of re-use including for commercial purposes, provided that author attribution and integrity are maintained (https://creativecommons.org/licenses/by/4.0/).
spellingShingle Chen, Zehua
Xue, Haibo
Brocks, Geert
Bobbert, Peter A.
Tao, Shuxia
Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title_full Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title_fullStr Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title_full_unstemmed Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title_short Thermodynamic Origin of the Photostability of the Two-Dimensional Perovskite PEA(2)Pb(I(1–x)Br(x))(4)
title_sort thermodynamic origin of the photostability of the two-dimensional perovskite pea(2)pb(i(1–x)br(x))(4)
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9926482/
https://www.ncbi.nlm.nih.gov/pubmed/36816777
http://dx.doi.org/10.1021/acsenergylett.2c02463
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