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In situ constructing atomic interface in ruthenium-based amorphous hybrid-structure towards solar hydrogen evolution.

Dong LiuTao DingLifeng WangHuijuan ZhangLi XuBeibei PangXiaokang LiuHuijuan WangJunhui WangKaifeng WuTao Yao
Published in: Nature communications (2023)
The rational steering and construction of efficient and stable atomic interfaces is highly desirable but rather challenging in solar energy conversion. Here, we report an in-situ oxygen impregnation strategy to build abundant atomic interfaces composed of homogeneous Ru and RuO x amorphous hybrid-mixture with ultrafast charge transfer, for solar hydrogen evolution with sacrificial agent free. Via in-situ synchrotron X-ray absorption and photoelectron spectroscopies, we can precisely track and identify the gradual formation of atomic interfaces towards homogeneous Ru-RuO x hybrid-structure at the atomic level. Benefiting from the abundant interfaces, the amorphous RuO x sites can intrinsically trap the photoexcited hole within an ultrafast process (<100 fs), and the amorphous Ru sites enable subsequent electron transfer (~1.73 ps). Hence, this hybrid-structure triggers long-lived charge-separated states, and results in a high hydrogen evolution rate of 60.8 μmol·h -1 . This design integrating the two sites fulfilled each half-reaction in a single hybrid-structure suggests potential guidelines towards efficient artificial photosynthesis.
Keyphrases
  • electron transfer
  • room temperature
  • energy transfer
  • electron microscopy
  • high resolution
  • risk assessment