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Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells
Wide band-gap perovskite solar cells have the potential for a relatively high output voltage and resilience in a degradation-inducing environment. Investigating the reasons why high voltages with adequate output power have not been realized yet is an underexplored part in perovskite research althoug...
Autores principales: | , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2020
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7746738/ https://www.ncbi.nlm.nih.gov/pubmed/33335234 http://dx.doi.org/10.1038/s41598-020-79348-1 |
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author | Ferdowsi, Parnian Ochoa-Martinez, Efrain Alonso, Sandy Sanchez Steiner, Ullrich Saliba, Michael |
author_facet | Ferdowsi, Parnian Ochoa-Martinez, Efrain Alonso, Sandy Sanchez Steiner, Ullrich Saliba, Michael |
author_sort | Ferdowsi, Parnian |
collection | PubMed |
description | Wide band-gap perovskite solar cells have the potential for a relatively high output voltage and resilience in a degradation-inducing environment. Investigating the reasons why high voltages with adequate output power have not been realized yet is an underexplored part in perovskite research although it is of paramount interest for multijunction solar cells. One reason is interfacial carrier recombination that leads to reduced carrier lifetimes and voltage loss. To further improve the V(oc) of methylammonium lead tri-bromide (MAPbBr(3)), that has a band-gap of 2.3 eV, interface passivation technique is an important strategy. Here we demonstrate two ultrathin passivation layers consisting of PCBM and PMMA, that can effectively passivate defects at the TiO(2)/perovskite and perovskite/spiro-OMeTAD interfaces, respectively. In addition, perovskite crystallization was investigated with the established anti-solvent method and the novel flash infrared annealing (FIRA) with and without passivation layers. These modifications significantly suppress interfacial recombination providing a pathway for improved V(OC)’s from 1.27 to 1.41 V using anti solvent and from 1.12 to 1.36 V using FIRA. Furthermore, we obtained more stable devices through passivation after 140 h where the device retained 70% of the initial performance value. |
format | Online Article Text |
id | pubmed-7746738 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2020 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-77467382020-12-18 Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells Ferdowsi, Parnian Ochoa-Martinez, Efrain Alonso, Sandy Sanchez Steiner, Ullrich Saliba, Michael Sci Rep Article Wide band-gap perovskite solar cells have the potential for a relatively high output voltage and resilience in a degradation-inducing environment. Investigating the reasons why high voltages with adequate output power have not been realized yet is an underexplored part in perovskite research although it is of paramount interest for multijunction solar cells. One reason is interfacial carrier recombination that leads to reduced carrier lifetimes and voltage loss. To further improve the V(oc) of methylammonium lead tri-bromide (MAPbBr(3)), that has a band-gap of 2.3 eV, interface passivation technique is an important strategy. Here we demonstrate two ultrathin passivation layers consisting of PCBM and PMMA, that can effectively passivate defects at the TiO(2)/perovskite and perovskite/spiro-OMeTAD interfaces, respectively. In addition, perovskite crystallization was investigated with the established anti-solvent method and the novel flash infrared annealing (FIRA) with and without passivation layers. These modifications significantly suppress interfacial recombination providing a pathway for improved V(OC)’s from 1.27 to 1.41 V using anti solvent and from 1.12 to 1.36 V using FIRA. Furthermore, we obtained more stable devices through passivation after 140 h where the device retained 70% of the initial performance value. Nature Publishing Group UK 2020-12-17 /pmc/articles/PMC7746738/ /pubmed/33335234 http://dx.doi.org/10.1038/s41598-020-79348-1 Text en © The Author(s) 2020 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. |
spellingShingle | Article Ferdowsi, Parnian Ochoa-Martinez, Efrain Alonso, Sandy Sanchez Steiner, Ullrich Saliba, Michael Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title | Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title_full | Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title_fullStr | Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title_full_unstemmed | Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title_short | Ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
title_sort | ultrathin polymeric films for interfacial passivation in wide band-gap perovskite solar cells |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7746738/ https://www.ncbi.nlm.nih.gov/pubmed/33335234 http://dx.doi.org/10.1038/s41598-020-79348-1 |
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