This is a page describing data taken during an experiment at the ISIS Neutron and Muon Source. Information about the ISIS Neutron and Muon Source can be found at https://www.isis.stfc.ac.uk.
Pressure and Temperature dependence of the CsPb(IxBr1-x)3 perovskites: candidate materials for stable and efficient solar cells.
Abstract: Halide perovskites have been the focus of an intense research effort, ever since the discovery that they can be employed to fabricate highly efficient solar cells. One of the key challenges is to produce materials that are chemically and structurally stable, yet have optimal optoelectronic properties. This effort is hampered by the almost complete lack of experimental data about their basic thermodynamic behaviour as a function of pressure and temperature - the ‘classic’ clean variables through which stability is tuned. Here we propose a neutron powder diffraction study as a function of pressure and temperature of the ‘fully-inorganic’ CsPb(IxBr1-x)3 perovskite - a promising alternative to the popular organic-inorganic ‘hybrids’. Key information obtained in this experiment will be later compared with first-principle calculations to define a route towards better materials properties.
Principal Investigator: Professor Paolo Radaelli
Experimenter: Dr Roger Johnson
Local Contact: Dr Ivan da Silva Gonzalez
Experimenter: Miss Laura Schade
Experimenter: Professor Henry Snaith
Experimenter: Ms Rebecca Sutton
DOI: 10.5286/ISIS.E.RB1820441
ISIS Experiment Number: RB1820441
Part DOI | Instrument | Public release date | Download Link |
---|---|---|---|
10.5286/ISIS.E.RB1820441-1 | GEM | 29 March 2022 | Download |
Publisher: STFC ISIS Neutron and Muon Source
Data format: RAW/Nexus
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Data Citation
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publication is as:
[author], [date], [title], [publisher],
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Professor Paolo Radaelli et al; (2019): Pressure and Temperature dependence of the CsPb(IxBr1-x)3 perovskites: candidate materials for stable and efficient solar cells. , STFC ISIS Neutron and Muon Source, https://doi.org/10.5286/ISIS.E.RB1820441
Data is released under the CC-BY-4.0 license.