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Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction
Journal of Materials Chemistry C, Volume: 8, Issue: 36, Pages: 12648 - 12655
Swansea University Author: James Durrant
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DOI (Published version): 10.1039/d0tc03390a
Abstract
Photoactive layer thickness is a key parameter for optimization of photovoltaic power conversion efficiency (PCE), yet its impact on charge extraction and recombination hasn’t been fully understood in perovskite solar cells (PSCs). Herein we find that in planar PSCs the perovskite thickness yielding...
Published in: | Journal of Materials Chemistry C |
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ISSN: | 2050-7526 2050-7534 |
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Royal Society of Chemistry (RSC)
2020
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URI: | https://cronfa.swan.ac.uk/Record/cronfa55400 |
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2021-08-29T14:45:19.0206363 v2 55400 2020-10-12 Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction f3dd64bc260e5c07adfa916c27dbd58a 0000-0001-8353-7345 James Durrant James Durrant true false 2020-10-12 EAAS Photoactive layer thickness is a key parameter for optimization of photovoltaic power conversion efficiency (PCE), yet its impact on charge extraction and recombination hasn’t been fully understood in perovskite solar cells (PSCs). Herein we find that in planar PSCs the perovskite thickness yielding maximal PCE is strongly light-intensity dependent. Whilst under 1 sun irradiation the PCE is relatively invariant for perovskite thicknesses between 250 to 750 nm, at lower light intensities (0.1–0.5 sun) the thickest devices yield strongly enhanced PCE, but at higher light intensities (>1 sun) the thinnest devices give optimal PCE. Our results unravel that increased perovskite thickness leads to enhanced light absorption, reduced interfacial recombination at open circuit but greater bimolecular recombination losses at short circuit thus is suitable for devices working under weak illumination, typical of many real-world applications. Reducing perovskite thickness, however, shows the contrast trend and is suitable for PSCs working under concentrated illumination. Journal Article Journal of Materials Chemistry C 8 36 12648 12655 Royal Society of Chemistry (RSC) 2050-7526 2050-7534 28 9 2020 2020-09-28 10.1039/d0tc03390a COLLEGE NANME Engineering and Applied Sciences School COLLEGE CODE EAAS Swansea University EPSRC, NRF EP/P032591/1, NRF-2017K1A1A2013153, EP/L016702/1 2021-08-29T14:45:19.0206363 2020-10-12T12:27:01.7555774 Faculty of Science and Engineering School of Engineering and Applied Sciences - Materials Science and Engineering Tian Du 1 Weidong Xu 2 Shengda Xu 3 Sinclair R. Ratnasingham 4 Chieh-Ting Lin 5 Jinhyun Kim 6 Joe Briscoe 7 Martyn A. McLachlan 8 James Durrant 0000-0001-8353-7345 9 55400__18408__99336e3c7f8e4edeacf88597513129c3.pdf 55400.pdf 2020-10-12T12:28:33.5182133 Output 4152550 application/pdf Version of Record true © 2020 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution -NonCommercial 3.0 Unported Licence true eng http://creativecommons.org/licenses/by-nc/3.0/ |
title |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
spellingShingle |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction James Durrant |
title_short |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
title_full |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
title_fullStr |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
title_full_unstemmed |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
title_sort |
Light-intensity and thickness dependent efficiency of planar perovskite solar cells: charge recombination versus extraction |
author_id_str_mv |
f3dd64bc260e5c07adfa916c27dbd58a |
author_id_fullname_str_mv |
f3dd64bc260e5c07adfa916c27dbd58a_***_James Durrant |
author |
James Durrant |
author2 |
Tian Du Weidong Xu Shengda Xu Sinclair R. Ratnasingham Chieh-Ting Lin Jinhyun Kim Joe Briscoe Martyn A. McLachlan James Durrant |
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Journal article |
container_title |
Journal of Materials Chemistry C |
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8 |
container_issue |
36 |
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12648 |
publishDate |
2020 |
institution |
Swansea University |
issn |
2050-7526 2050-7534 |
doi_str_mv |
10.1039/d0tc03390a |
publisher |
Royal Society of Chemistry (RSC) |
college_str |
Faculty of Science and Engineering |
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Faculty of Science and Engineering |
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School of Engineering and Applied Sciences - Materials Science and Engineering{{{_:::_}}}Faculty of Science and Engineering{{{_:::_}}}School of Engineering and Applied Sciences - Materials Science and Engineering |
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description |
Photoactive layer thickness is a key parameter for optimization of photovoltaic power conversion efficiency (PCE), yet its impact on charge extraction and recombination hasn’t been fully understood in perovskite solar cells (PSCs). Herein we find that in planar PSCs the perovskite thickness yielding maximal PCE is strongly light-intensity dependent. Whilst under 1 sun irradiation the PCE is relatively invariant for perovskite thicknesses between 250 to 750 nm, at lower light intensities (0.1–0.5 sun) the thickest devices yield strongly enhanced PCE, but at higher light intensities (>1 sun) the thinnest devices give optimal PCE. Our results unravel that increased perovskite thickness leads to enhanced light absorption, reduced interfacial recombination at open circuit but greater bimolecular recombination losses at short circuit thus is suitable for devices working under weak illumination, typical of many real-world applications. Reducing perovskite thickness, however, shows the contrast trend and is suitable for PSCs working under concentrated illumination. |
published_date |
2020-09-28T02:13:05Z |
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1821369785621938176 |
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11.04748 |