Boosted Photothermal Catalytic Hydrogen Evolution in TiO₂/Bi₂Te₃ Systems via Controlled Transformation of Bi–Te Phonon-Glass to Bi–Te–O Glass
Date
2025
Authors
Motoki, S.
Zhang, J.
Lin, J.
Hu, K.
Ren, S.
Duan, X.
Wang, S.
Editors
Advisors
Journal Title
Journal ISSN
Volume Title
Type:
Journal article
Citation
Energy & Fuels, 2025; 39(35):17038-17048
Statement of Responsibility
Seiya Motoki, Jinqiang Zhang, Jingkai Lin, Kunsheng Hu, Shiying Ren, Xiaoguang Duan, and Shaobin Wang
Conference Name
Abstract
Photothermal catalysis has shown great promise for efficient water splitting toward green hydrogen production for its unique capability to convert sunlight into energetic hot carriers and localized thermal energy. However, suitable catalyst systems that fully exploit these effects remain limited. Phonon glass materials such as Bi₂Te₃ offer a broad spectrum of light absorption, making them attractive photothermal promoters, yet they contribute minimally to hot carrier generation. In this study, we explored the transformation of Bi₂Te₃ into Bi−Te−O glass phases and leveraged their photothermal/excitonic synergy, where thermal energy accelerates surface kinetics and excitonic species supply reactive charge carriers, by integrating them with TiO₂ to promote photothermal catalytic performance. Engineering thermal treatment at varying temperatures, we developed a TiO₂/Bi₂Te₃/Bi₂Te₄O₁₁ composite that achieved an optimized balance between photothermal and excitonic properties. Structural, optical, and surface analyses reveal that this balance is critical to achieving a hydrogen evolution rate of 2572 μmol h⁻¹ g⁻¹, nearly 10-fold higher than that of pristine TiO₂ (268 μmol h⁻¹ g⁻¹). These findings demonstrate a novel phase-engineering strategy for Bi2Te3-based hybrids, offering a dual approach via thermal and electronic pathways to guide the rational design of next-generation photothermal catalysts for solar fuel production.
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Dissertation Note
Provenance
Description
Published as part of Energy & Fuels special issue “2025 Energy and Fuels Rising Stars”.
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© 2025 American Chemical Society