Mapping the polymorphic phase transformations of CsPbI3 perovskite thin films

Abstract

Inorganic perovskite CsPbI3 has a bandgap of 1.7 eV, making it an ideal complementary absorber to Si for integration into tandem solar cells. However, the black, photoactive CsPbI3 phases are metastable and readily transform into a yellow non-perovskite δ-CsPbI3 phase at room temperature, posing a significant challenge to long-term device stability. In this study, we investigate the temperature-dependent dynamics of these phase transitions in CsPbI3 thin films using a combination of in situ X-ray diffraction and time-resolved optical microscopy. We find the transformation rate to be highly temperature-dependent, with the fastest conversion occurring at 225 °C, where 50% of the film transformed to δ-CsPbI3 within 17 minutes. To identify processing temperatures with longer phase-stability windows, we used the time- and temperature-dependent phase dynamics data to generate a time-temperature-transformation diagram for thin film CsPbI3. Processing near the peak conversion temperature must be completed within two minutes to retain black-phase purity, while processing above 280 °C or below 150 °C provides a much wider processing window with <1% conversion to δ-CsPbI3 occurring after 10 minutes. Conversely, it may be useful to hold CsPbI3 solar cells or thin films with phase-stabilizing modifications near 225 °C to accelerate potential phase transitions and maximally stress their stability.

Graphical abstract: Mapping the polymorphic phase transformations of CsPbI3 perovskite thin films

Supplementary files

Article information

Article type
Paper
Submitted
14 Mar 2025
Accepted
20 Aug 2025
First published
21 Aug 2025
This article is Open Access
Creative Commons BY-NC license

J. Mater. Chem. C, 2025, Advance Article

Mapping the polymorphic phase transformations of CsPbI3 perovskite thin films

R. Holley III, Q. C. Burlingame and Y. Loo, J. Mater. Chem. C, 2025, Advance Article , DOI: 10.1039/D5TC01126D

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