Please use this identifier to cite or link to this item: http://hdl.handle.net/1942/33814
Title: The role of spin in the degradation of organic photovoltaics
Authors: Ramirez, Ivan
Privitera, Alberto
Karuthedath, Safakath
Jungbluth, Anna
Benduhn, Johannes
Sperlich, Andreas
SPOLTORE, Donato 
VANDEWAL, Koen 
Laquai, Frederic
Riede, Moritz
Issue Date: 2021
Publisher: NATURE RESEARCH
Source: Nature Communications, 12 (1) (Art N° 471)
Abstract: Stability is now a critical factor in the commercialization of organic photovoltaic (OPV) devices. Both extrinsic stability to oxygen and water and intrinsic stability to light and heat in inert conditions must be achieved. Triplet states are known to be problematic in both cases, leading to singlet oxygen production or fullerene dimerization. The latter is thought to proceed from unquenched singlet excitons that have undergone intersystem crossing (ISC). Instead, we show that in bulk heterojunction (BHJ) solar cells the photo-degradation of C-60 via photo-oligomerization occurs primarily via back-hole transfer (BHT) from a charge-transfer state to a C-60 excited triplet state. We demonstrate this to be the principal pathway from a combination of steady-state optoelectronic measurements, time-resolved electron paramagnetic resonance, and temperature-dependent transient absorption spectroscopy on model systems. BHT is a much more serious concern than ISC because it cannot be mitigated by improved exciton quenching, obtained for example by a finer BHJ morphology. As BHT is not specific to fullerenes, our results suggest that the role of electron and hole back transfer in the degradation of BHJs should also be carefully considered when designing stable OPV devices. The commercialisation of organic photovoltaic technology calls for research on material degradation mechanisms. Ramirez et al. show that triplet excitons produced by back charge transfer can significantly impact the photo-stability of fullerene-based devices even in the absence of water and oxygen.
Notes: Ramirez, I (corresponding author), Heliatek GmbH, Treidlerstr 3, D-01139 Dresden, Germany.; Riede, M (corresponding author), Univ Oxford, Dept Phys, Clarendon Lab, Parks Rd, Oxford OX1 3PU, England.
ivan.ramirez@heliatek.com; moritz.riede@physics.ox.ac.uk
Other: Ramirez, I (corresponding author), Heliatek GmbH, Treidlerstr 3, D-01139 Dresden, Germany. Riede, M (corresponding author), Univ Oxford, Dept Phys, Clarendon Lab, Parks Rd, Oxford OX1 3PU, England. ivan.ramirez@heliatek.com; moritz.riede@physics.ox.ac.uk
Document URI: http://hdl.handle.net/1942/33814
e-ISSN: 2041-1723
DOI: 10.1038/s41467-020-20601-6
ISI #: WOS:000613566500006
Rights: The Author(s) 2021. 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 license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license 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 license, visit http://creativecommons.org/ licenses/by/4.0/
Category: A1
Type: Journal Contribution
Validations: ecoom 2022
Appears in Collections:Research publications

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