Extending the defect tolerance of halide perovskite nanocrystals to hot carrier cooling dynamics
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Defect tolerance is a critical enabling factor for efficient lead-halide perovskite materials, but the current understanding is primarily on band-edge (cold) carriers, with significant debate over whether hot carriers can also exhibit defect tolerance. Here, this important gap in the field is addressed by investigating how intentionally-introduced traps affect hot carrier relaxation in CsPbX3 nanocrystals (X = Br, I, or mixture). Using femtosecond interband and intraband spectroscopy, along with energy-dependent photoluminescence measurements and kinetic modelling, it is found that hot carriers are not universally defect tolerant in CsPbX3, but are strongly correlated to the defect tolerance of cold carriers, requiring shallow traps to be present (as in CsPbI3). It is found that hot carriers are directly captured by traps, instead of going through an intermediate cold carrier, and deeper traps cause faster hot carrier cooling, reducing the effects of the hot phonon bottleneck and Auger reheating. This work provides important insights into how defects influence hot carriers, which will be important for designing materials for hot carrier solar cells, multiexciton generation, and optical gain media.
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Acknowledgements: J.Y. and R.L.Z.H. acknowledge support from a UK Research and Innovation (UKRI) Frontier Grant (no. EP/X029900/1), awarded via the European Research Council Starting Grant 2021 scheme. J.Y. also gives thanks to Cambridge Philosophical Society for the Research Studentship Grant and Churchill College for various travel and research grants. N.M. and A.A.B. acknowledge support from the European Commission through the Marie Skłodowska-Curie Actions Project (PeroVIB, H2020-MSCA-IF-2020-101018002). Y.W.Z. acknowledges funding from the National Natural Science Foundation of China under Grant No. 12304036, the Open Project of Guangdong Provincial Key Laboratory of Magnetoelectric Physics and Devices (No. 2022B1212010008), the Guangdong Basic and Applied Basic Research Foundation (2023A1515010071), the Guangzhou Basic and Applied Basic Research Foundation (SL2022A04J00048), and the Fundamental Research Funds for the Central Universities, Sun Yat-sen University (23xkjc016). S.D.S., L.D. and J.M. acknowledge funding support from the European Research Council under the European Union’s Horizon 2020 research and innovation programme (HYPERION, 756962; PEROVSCI, 957513). J.M. acknowledges funding from a Marie Sklodowska-Curie Postdoctoral Fellowship via UKRI Horizon Europe Guarantee (grant number EP/X025764/1). S.D.S. thanks the Royal Society and Tata Group (UF150033). L.D. thanks the Cambridge Trusts and the China Scholarship Council for funding. J.M. acknowledges funding from Marie Sklodowska-Curie Postdoctoral Fellowships via UKRI Horizon Europe Guarantee (no. EP/X025764/1) and the National Natural Science Foundation of China (no. 62204049). L.v.T. thanks the Winton Programme for the Physics of Sustainability and the Engineering and Physical Sciences Research Council for funding. A.A.B. acknowledges support from the Royal Society and Leverhulme Trust. L.P. acknowledges support from the Spanish Ministerio de Ciencia e Innovación through Ramón y Cajal grant (grant no. RYC2018-026103-I), the Spanish State Research Agency (grant nos. PID2020-117371RA-I00 and TED2021-131628A-I00), and a grant from the Xunta de Galicia (grant no. ED431F2021/05). Y.-T.H. and R.L.Z.H. thank the Engineering and Physical Sciences Research Council (EPSRC, grant no. EP/V014498/2). R.L.Z.H. thanks the Royal Academy of Engineering through the Research Fellowships scheme (no. RF\201718\17101), as well as the Centre of Advanced Materials for Integrated Energy Systems (CAM-IES; EPSRC grant no. EP/T012218/1). The authors thank Dr. Mark Isaacs for XPS measurements. The author also would like to acknowledge that the X-ray photoelectron (XPS) data was acquired at the EPSRC National Facility for XPS (“HarwellXPS”, EP/Y023587/1, EP/Y023609/1, EP/Y023536/1, EP/Y023552/1 and EP/Y023544/1; these are associated with Dr. Mark Isaacs).
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European Commission (EC) (H2020-MSCA-IF-2020-101018002)
National Natural Science Foundation of China (National Science Foundation of China) (12304036)

