Twinned crystal Cd 0.9 Zn 0.1 S/MoO 3 nanorod S-scheme heterojunctions as promising photocatalysts for efficient hydrogen evolution

Leveraging solar energy through photocatalytic hydrogen production from water stands out as one of the most promising approaches to address the energy and environmental challenges. The choice of catalyst profoundly influences the outcomes of photocatalytic reactions, and constructing heterojunctions...

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Veröffentlicht in:Dalton transactions : an international journal of inorganic chemistry 2024-05, Vol.53 (20), p.8781-8790
Hauptverfasser: Chen, Jie, Xie, Ying, Yu, Haitao, Li, Zhenzi, Zhou, Wei
Format: Artikel
Sprache:eng
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Zusammenfassung:Leveraging solar energy through photocatalytic hydrogen production from water stands out as one of the most promising approaches to address the energy and environmental challenges. The choice of catalyst profoundly influences the outcomes of photocatalytic reactions, and constructing heterojunctions has emerged as a widely applied strategy to overcome the limitations associated with single-phase photocatalysts. MoO , renowned for its high chemical stability, encounters issues such as low photocatalytic efficiency and fast recombination of photogenerated electrons and holes. To tackle these challenges, the morphology of MoO has been controlled to form nanorods, simultaneously suppressing the aggregation of the catalyst and increasing the number of surface-active sites. Moreover, to facilitate the separation of photogenerated charge carriers, Cd Zn S nanoparticles with a twin crystal structure are deposited on the surface of MoO , establishing an S-scheme heterojunction. Experimental findings demonstrate that the synergistic effects arising from the well-defined morphology and interface interactions extend the absorption range to visible light response, improve charge transfer activity, and prolong the lifetime of charge carriers. Consequently, Cd Zn S/MoO S-scheme heterojunctions exhibit outstanding photocatalytic hydrogen production performance (3909.79 μmol g h ) under visible light irradiation, surpassing that of MoO by nearly nine fold.
ISSN:1477-9226
1477-9234
DOI:10.1039/d4dt00585f