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Differences in photoinduced optical transients in perovskite absorbers for solar cells

Methylammonium lead iodide films and powdered crystals were studied by time-resolved absorption and emission spectroscopy on the time scales from femtoseconds to nanoseconds. Strikingly different transient absorption signals were observed, changing from strong long-wavelength band-edge bleach to wea...

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Autores principales: Pydzińska, Katarzyna, Karolczak, Jerzy, Szafrański, Marek, Ziółek, Marcin
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Royal Society of Chemistry 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9078339/
https://www.ncbi.nlm.nih.gov/pubmed/35540378
http://dx.doi.org/10.1039/c8ra00579f
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author Pydzińska, Katarzyna
Karolczak, Jerzy
Szafrański, Marek
Ziółek, Marcin
author_facet Pydzińska, Katarzyna
Karolczak, Jerzy
Szafrański, Marek
Ziółek, Marcin
author_sort Pydzińska, Katarzyna
collection PubMed
description Methylammonium lead iodide films and powdered crystals were studied by time-resolved absorption and emission spectroscopy on the time scales from femtoseconds to nanoseconds. Strikingly different transient absorption signals were observed, changing from strong long-wavelength band-edge bleach to weak signatures of band-shift, which depended on the absorber form (films or polycrystals) and preparation method (stoichiometric or non-stoichiometric). The observed differences were correlated with the variation in absorption and emission spectra, changes in photo-induced carrier lifetimes and solar cell efficiency. These differences also pointed out that similar perovskite absorbers can provide significantly different transient responses and emphasize that special care must be taken when interpolating the obtained findings to the processes occurring in the most efficient devices.
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spelling pubmed-90783392022-05-09 Differences in photoinduced optical transients in perovskite absorbers for solar cells Pydzińska, Katarzyna Karolczak, Jerzy Szafrański, Marek Ziółek, Marcin RSC Adv Chemistry Methylammonium lead iodide films and powdered crystals were studied by time-resolved absorption and emission spectroscopy on the time scales from femtoseconds to nanoseconds. Strikingly different transient absorption signals were observed, changing from strong long-wavelength band-edge bleach to weak signatures of band-shift, which depended on the absorber form (films or polycrystals) and preparation method (stoichiometric or non-stoichiometric). The observed differences were correlated with the variation in absorption and emission spectra, changes in photo-induced carrier lifetimes and solar cell efficiency. These differences also pointed out that similar perovskite absorbers can provide significantly different transient responses and emphasize that special care must be taken when interpolating the obtained findings to the processes occurring in the most efficient devices. The Royal Society of Chemistry 2018-02-09 /pmc/articles/PMC9078339/ /pubmed/35540378 http://dx.doi.org/10.1039/c8ra00579f Text en This journal is © The Royal Society of Chemistry https://creativecommons.org/licenses/by/3.0/
spellingShingle Chemistry
Pydzińska, Katarzyna
Karolczak, Jerzy
Szafrański, Marek
Ziółek, Marcin
Differences in photoinduced optical transients in perovskite absorbers for solar cells
title Differences in photoinduced optical transients in perovskite absorbers for solar cells
title_full Differences in photoinduced optical transients in perovskite absorbers for solar cells
title_fullStr Differences in photoinduced optical transients in perovskite absorbers for solar cells
title_full_unstemmed Differences in photoinduced optical transients in perovskite absorbers for solar cells
title_short Differences in photoinduced optical transients in perovskite absorbers for solar cells
title_sort differences in photoinduced optical transients in perovskite absorbers for solar cells
topic Chemistry
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9078339/
https://www.ncbi.nlm.nih.gov/pubmed/35540378
http://dx.doi.org/10.1039/c8ra00579f
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