Synchronizing periodic excitations of photocatalysts with a Michelson interferometer on operando FT–IR spectroscopy, researchers led by Toshiki Sugimoto succeeded in observing and identifying the reactive electron species for photocatalytic hydrogen evolution. In contrast to previous assumptions, this study demonstrates that it is not the free electrons in metal cocatalysts but the electrons trapped in the periphery of cocatalysts that directly contribute to the photocatalysis.
The findings are published in the Journal of the American Chemical Society.
Since the discovery of photoelectrochemical hydrogen evolution by Honda and Fujishima in 1972, heterogeneous photocatalysis has been intensively investigated and is still a hot topic in science and technology. In particular, understanding of reactive electron species and active reaction sites on photocatalytic reduction reaction are vital for designing and manufacturing innovative catalysts with improved evolution activity of hydrogen as a sustainable energy carrier.
However, despite its fundamental importance, microscopic understanding of photocatalysis remains a highly challenging issue owing to an inherent difficulty in experimentally observing and extracting weak spectroscopic signals originating from the photoexcited reactive electron species.
This is predominantly due to the inevitable temperature increment for catalyst samples under actual photocatalytic reaction conditions upon continuous photon irradiation. In this case, the weak signals derived from reactive photoexcited electron species are readily overwhelmed by intense background signals originating from thermally excited nonreactive electrons.
Researchers (Dr. Hiromasa Sato and Prof. Toshiki Sugimoto) at the Institute for Molecular Science, The Graduate University for Advanced Studies, SOKENDAI succeeded in significantly suppressing the signals derived from thermally excited electrons and observing the reactive photogenerated electrons contributing to the photocatalytic hydrogen evolution.
This innovation was achieved by a new method based on synchronization of the millisecond periodic excitations of photocatalysts with a Michelson interferometer used for FT–IR spectroscopy. This demonstration was achieved with metal-loaded oxide photocatalysts under steam methane reforming and water splitting conditions.
Although it has long been conventionally believed that loaded metal cocatalysts function as sinks for reactive photogenerated electrons and active sites for reduction reactions, they found that the free electron species in the metal cocatalysts were not directly involved in the photocatalytic reduction reaction. Alternatively, the electrons shallowly trapped in the in-gap states of oxides contributed to enhancing the hydrogen evolution rate upon the loading of metal cocatalysts.
The electron abundance in the in-gap states, especially metal-induced semiconductor surface states, was clearly correlated to the reaction activity, suggesting that such metal-induced semiconductor surface states formed in the periphery of the metal cocatalyst play key roles in the photocatalytic hydrogen evolution.
These microscopic insights shift a paradigm on the traditionally believed role of metal cocatalysts in photocatalysis and provide a fundamental basis for rational design of the metal/oxide complex interfaces as promising platforms for nonthermal hydrogen evolution.
Furthermore, the new approach of operando infrared spectroscopy is widely applicable to other catalytic reaction systems and materials driven by the aid of photons and/or external electric field/potential. Therefore, the new approach could have great potential to uncover hidden key factors to enhance catalyst performance.
More information:
Hiromasa Sato et al, Direct Operando Identification of Reactive Electron Species Driving Photocatalytic Hydrogen Evolution on Metal-Loaded Oxides, Journal of the American Chemical Society (2024). DOI: 10.1021/jacs.3c14558
Provided by
National Institutes of Natural Sciences
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Spectroscopy study reveals electrons in cocatalyst periphery drive photocatalytic hydrogen evolution (2024, August 29)
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