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The impact of interfacial quality and nanoscale performance disorder on the stability of alloyed perovskite solar cells

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Abstract

Microscopy provides a proxy for assessing the operation of perovskite solar cells, yet most works in the literature have focused on bare perovskite thin films, missing charge transport and recombination losses present in full devices. Here we demonstrate a multimodal operando microscopy toolkit to measure and spatially correlate nanoscale charge transport losses, recombination losses and chemical composition. By applying this toolkit to the same scan areas of state-of-the-art, alloyed perovskite cells before and after extended operation, we show that devices with the highest macroscopic performance have the lowest initial performance spatial heterogeneity—a crucial link that is missed in conventional microscopy. We show that engineering stable interfaces is critical to achieving robust devices. Once the interfaces are stabilized, we show that compositional engineering to homogenize charge extraction and to minimize variations in local power conversion efficiency is critical to improve performance and stability. We find that in our device space, perovskites can tolerate spatial disorder in chemistry, but not charge extraction.

Description

Acknowledgements: K.F. acknowledges an Engineering and Physical Sciences Research Council (EPSRC) Doctoral Prize Postdoctoral Fellowship, George and Lilian Schiff Studentship, Winton Sustainability Fund Studentship and an EPSRC studentship. C.C. acknowledges the support of a Marshall Scholarship and Winton Sustainability Fund Studentship. We acknowledge the Diamond Light Source (Didcot, Oxfordshire, UK) for providing beamtime at the I14 Hard X-ray Nanoprobe facility through proposal MG30427 and MG31964. M.A. acknowledges support from the Royal Academy of Engineering under the Research Fellowship programme and from MICIU/AEI/10.13039/501100011033 and the European Union NextGeneration EU/PRTR through a Ramón y Cajal Fellowship (RYC2021-034941-I). S.D.S. acknowledges the Royal Society and Tata Group (UF150033). Funding for A.A.-A., F.S., L.Z. and S.A. was provided by the Federal Ministry of Education and Research (BMBF) through the project PEROWIN (grant number 03SF0631) and by the Helmholtz Association within the projects HySPRINT Innovation lab, the EU Partnering project TAPAS and the project ‘Zeitenwende – Tandem Solarzellen’. T.A.S. acknowledges funding from EPSRC Cambridge NanoDTC, EP/S022953/1. M.D. acknowledges UKRI guarantee funding for Marie Sklodowska-Curie Actions Postdoctoral Fellowships 2022 (EP/Y024648/1). The work has received funding from the European Research Council under the European Union’s Horizon 2020 research and innovation programme (HYPERION–grant agreement number 756962). We acknowledge the EPSRC (EP/R023980/1 and EP/T02030X/1) for funding. We acknowledge R.A. Belisle, S. Macpherson, T. Schloemer and M. Merchant for helpful discussion and comments on the manuscript. We acknowledge E. Choi for assistance with synchrotron measurements. For the purpose of open access, we have applied a Creative Commons Attribution (CC BY) licence to any author accepted manuscript version arising from this submission.

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Journal Title

Nature Energy

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Journal ISSN

2058-7546

Volume Title

10

Publisher

Nature Publishing Group UK

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Except where otherwised noted, this item's license is described as http://creativecommons.org/licenses/by/4.0/
Sponsorship
EC | EU Framework Programme for Research and Innovation H2020 | H2020 Priority Excellent Science | H2020 European Research Council (H2020 Excellent Science - European Research Council) (756962, 756962, 756962, 756962, 756962)
Royal Academy of Engineering (Research Fellowship, Research Fellowship)
Bundesministerium für Bildung und Forschung (Federal Ministry of Education and Research) (03SF0631, 03SF0631, 03SF0631, 03SF0631, 03SF0631)
RCUK | Engineering and Physical Sciences Research Council (EPSRC) (EP/T02030X/1, Doctoral Prize Fellowship, Doctoral Prize Fellowship, EP/S022953/1)