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Boosting Solar‐Driven CO<sub>2</sub> Conversion to Ethanol via Single‐Atom Catalyst with Defected Low‐Coordination Cu‐N<sub>2</sub> Motif

68

Citations

58

References

2024

Year

Abstract

Cu-based catalysts have been shown to selectively catalyze CO<sub>2</sub> photoreduction to C<sub>2+</sub> solar fuels. However, they still suffer from poor activity and low selectivity. Herein, we report a high-performance carbon nitride supported Cu single-atom catalyst featuring defected low-coordination Cu-N<sub>2</sub> motif (Cu-N<sub>2</sub>-V). Lead many recently reported photocatalysts and its Cu-N<sub>3</sub> and Cu-N<sub>4</sub> counterparts, Cu-N<sub>2</sub>-V exhibits superior photocatalytic activity for CO<sub>2</sub> reduction to ethanol and delivers 69.8 μmol g<sup>-1</sup> h<sup>-1</sup> ethanol production rate, 97.8 % electron-based ethanol selectivity, and a yield of ~10 times higher than Cu-N<sub>3</sub> and Cu-N<sub>4</sub>. Revealed by the extensive experimental investigation combined with DFT calculations, the superior photoactivity of Cu-N<sub>2</sub>-V stems from its defected Cu-N<sub>2</sub> configuration, in which the Cu sites are electron enriched and enhance electron delocalization. Importantly, Cu in Cu-N<sub>2</sub>-V exist in both Cu<sup>+</sup> and Cu<sup>2+</sup> valence states, although predominantly as Cu<sup>+</sup>. The Cu<sup>+</sup> sites support the CO<sub>2</sub> activation, while the co-existence of Cu<sup>+</sup>/Cu<sup>2+</sup> sites are highly conducive for strong *CO adsorption and subsequent *CO-*CO dimerization enabling C-C coupling. Furthermore, the hollow microstructure of the catalyst also promotes light adsorption and charge separation efficiency. Collectively, these make Cu-N<sub>2</sub>-V an effective and high-performance catalyst for the solar-driven CO<sub>2</sub> conversion to ethanol. This study also elucidates the C-C coupling reaction path via *CO-*CO to *COCOH and rate-determining step, and reveals the valence state change of partial Cu species from Cu<sup>+</sup> to Cu<sup>2+</sup> in Cu-N<sub>2</sub>-V during CO<sub>2</sub> photoreduction reaction.

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