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Operando insights into stability of perovskite-based solar water splitting devices
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  • Published: 26 January 2026

Operando insights into stability of perovskite-based solar water splitting devices

  • Chang-Seop Jeong1 na1,
  • Wooyong Jeong1 na1,
  • Juwon Yun1 na1,
  • Donyoung Kang  ORCID: orcid.org/0000-0003-2680-74892,
  • Byungjun Kang  ORCID: orcid.org/0000-0001-7220-801X2,
  • Hyungsoo Lee  ORCID: orcid.org/0000-0003-1858-70091,
  • Jun Hwan Kim1,
  • Hyungsuk Lee  ORCID: orcid.org/0000-0002-7873-71632 &
  • …
  • Jooho Moon  ORCID: orcid.org/0000-0002-6685-99991 

Nature Communications , Article number:  (2026) Cite this article

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Subjects

  • Electrocatalysis
  • Hydrogen energy
  • Photocatalysis
  • Solar cells

Abstract

Perovskite-based solar water splitting systems are promising candidates for addressing environmental challenges, exceeding the commercialization efficiency of solar-to-hydrogen (STH) at >10%. However, the operational stability remains suboptimal due to insufficient in situ/operando insights into charge carrier dynamics. Here, we investigate the role of charge accumulation on operational stability through operando catalytic modulation via near-infrared (NIR) toggling on a photothermal catalyst. Electrochemical analyses under operando NIR toggling demonstrate enhanced hydrogen evolution reaction kinetics and reduced charge recombination. In situ analyses confirm that reduced charge accumulation suppresses ion migration in the perovskite layer, thereby enhancing operational stability. The NIR-irradiated cathode delivers a photocurrent density of 25.48 mA cm–2, maintaining 90% of its initial photocurrent density at 0 VRHE for 310 h. A parallelly-illuminated coplanar system with NIR-irradiated perovskite-based water splitting cathode operates without bias, achieving a STH efficiency of 15.18%, retaining 70% of their initial performance for 115 h.

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Data availability

All data generated in this study are provided in the Source Data file. Source data are provided with this paper.

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Acknowledgements

This research was supported by National R&D Program through the National Research Foundation (NRF) of Korea (No. 2021R1A3B1068920 and 2021M3H4A1A03049662) funded by the Ministry of Science and ICT. This research was also supported by the Yonsei Signature Research Cluster Program of 2021 (2021-22-0002) and the Yonsei Fellowship, funded by Lee Youn Jae.

Author information

Author notes
  1. These authors contributed equally: Chang-Seop Jeong, Wooyong Jeong, Juwon Yun.

Authors and Affiliations

  1. Department of Materials Science and Engineering, Yonsei University, 50, Yonsei-ro, Seodaemun-gu, Seoul, Republic of Korea

    Chang-Seop Jeong, Wooyong Jeong, Juwon Yun, Hyungsoo Lee, Jun Hwan Kim & Jooho Moon

  2. School of Mechanical Engineering, Yonsei University, 50, Yonsei-ro, Seodaemun-gu, Seoul, Republic of Korea

    Donyoung Kang, Byungjun Kang & Hyungsuk Lee

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  1. Chang-Seop Jeong
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Contributions

C.-S.J. and J.M. conceived the idea and designed the cathode. C.-S.J., W.J., and J.Y. fabricated the perovskite-based electrodes and wrote the initial draft. W.J. and J.Y. conducted in-situ Raman spectroscopy and DLCP measurements, while J.Y. and C.-S.J. performed IMVS/IMPS tests and collected ex-situ data. C.-S.J. and W.J. analyzed the operando electrochemical data, and B.K. and C.-S.J. carried out high-speed profiling of bubble dynamics. D.K. and B.K. developed FEM modeling of Marangoni convection, with Hyungsoo L. and J.H.K. preparing the experimental setup. C.-S.J., W.J., J.W., B.K., D.K., Hyungsoo L., J.H.K., Hyungsuk L., and J.M. contributed to the discussion and revision of the manuscript. J.M. supervised the overall project.

Corresponding author

Correspondence to Jooho Moon.

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Nature Communications thanks Jingshan Luo and the other anonymous reviewer(s) for their contribution to the peer review of this work. A peer review file is available.

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Jeong, CS., Jeong, W., Yun, J. et al. Operando insights into stability of perovskite-based solar water splitting devices. Nat Commun (2026). https://doi.org/10.1038/s41467-026-68357-9

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  • Received: 27 May 2025

  • Accepted: 05 January 2026

  • Published: 26 January 2026

  • DOI: https://doi.org/10.1038/s41467-026-68357-9

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