Abstract
Ammonia (NH3) splitting to hydrogen (H2) is a promising route for on-site production of green hydrogen energy; however, the application is limited due to high-cost noble-metal-based catalysts and high operating temperature of the endothermic nature. Herein, we develop a series of macroporous carbon nitride-supported single-atom transition metal (TMs-MCN, TMs: Co, Mn, Fe, Ni, Cu) catalyst panels for solar light-driven photocatalytic gaseous NH3 splitting. Under ambient reaction conditions, the optimized Ni-MCN shows an H2 production rate of 35.6 μmol g-1 h-1, much superior to that of MCN and other TMs-MCN. Such enhanced photoactivity is attributed to the presence of Ni-N4 sites, which improve the optical properties, accelerate charge carrier separation/transfer, and boost NH3 splitting kinetics of the catalysts. Density functional theory calculations further reveal that the Ni-N4 sites can effectively modify the electronic structure of the carbon nitride. Compared with other metal sites, the Ni-N4 site possesses moderate NH3 binding strength and the lowest energy barrier to facilitate the formation of key intermediates *NH + *H. These findings provide valuable guidelines for the rational design of single-atom catalysts toward energy- and cost-effective photocatalytic NH3 splitting for H2 production.
| Original language | English |
|---|---|
| Pages (from-to) | 11711-11722 |
| Number of pages | 12 |
| Journal | ACS Catalysis |
| Volume | 13 |
| Issue number | 17 |
| DOIs | |
| Publication status | Published - 2023 |
Funding
| Funders | Funder number |
|---|---|
| ARC Australian Research Council | DE220101074, DP200103206 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 7 Affordable and Clean Energy
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