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.