To improve the photocatalytic activities of narrow band gap oxide semiconductors for H 2 evolution under solar irradiation, it is highly desired to develop effective acceptors for visible light-excited high-energy-level electrons. Herein, we have successfully fabricated Ag-modified TiO 2 /BiVO 4 nanocomposites by putting nanosized BiVO 4 into the Ag modified TiO 2 sol. Both steady-state and transient-statesurface photovoltage spectra demonstrate that photogenerated charge separation and lifetime of nanosized BiVO 4 is promoted when coupling with TiO 2 and modifying an appropriate amount of Ag, while the lifetime of photogenerated electrons got prolonged. Interestingly, the resulting Ag-TiO 2 /BiVO 4 nanocomposites exhibit excellent visible light activities for H 2 evolution, although the visible light activities of TiO 2 /BiVO 4 one, Ag/BiVO 4 and bare BiVO 4 are neglectable, indicating that AgTiO 2 could be utilized as effective acceptors for hydrogen production. It is suggested based on the experimental data that the effective acceptors be attributed to the used TiO 2 for accepting the high-energy-level electrons generated from BiVO 4 and to the modified Ag for being reduced then to catalyze H 2 -evolution reactions. The developed strategy is versatile for other narrow band gap semiconductors, like WO 3 and Fe 2 O 3 .
■ INTRODUCTIONPhotocatalytic hydrogen evolution is regarded as a potential technique that can solve the current increasingly serious energy crisis through effective solar utilization. 1 Despite a great deal of effort made, the quantum efficiencies of state-of-art works are still low, far from the practical requirement for industrialization. 2,3 Photocatalytic reactions for H 2 evolution are mainly involved with complex thermodynamics and kinetic processes. In general, efficient photocatalysts are needed to possess strong solar-light absorption, high charge separation and superior catalytic capacity. It is well-known that cheap, stable, and environment friendly narrow band gap oxide semiconductors, such as BiVO 4 , Fe 2 O 3 , and WO 3 , can greatly absorb solar light, and the electrons will be excited from valence band (VB) to conduction band (CB) bottom and even over the level under solar irradiation. 4−6 The excited electrons at much higher energy level than the CB bottom usually relax to the CB bottom quite quickly (within picosecond time scale). 7,8 Since their CB bottom levels are usually located below 0 eV versus NHE, 9 so that the excited electrons are not suitable for energetic H 2 evolution, it is understandable that such narrowband gap oxides always exhibit low photocatalytic activities. However, it is worth noting that those visible-light-excited highenergy-level (HEL) electrons would naturally possess strong capacity to induce reduction reactions with water molecules thermodynamically. 10,11 For this, the key would be how to prolong the lifetimes of HEL electrons by altering the fast relaxation process. Unfortunately, it has seldom been reported until now.Constructing a heterojuntional ...