| Literature DB >> 30996901 |
Hao Lyu1, Takashi Hisatomi2, Yosuke Goto1, Masaaki Yoshida3,4, Tomohiro Higashi1, Masao Katayama1, Tsuyoshi Takata2, Tsutomu Minegishi1, Hiroshi Nishiyama1, Taro Yamada1, Yoshihisa Sakata3, Kiyotaka Asakura5, Kazunari Domen1,2.
Abstract
Photocatalytic water splitting is a viable approach to the large-scale production of renewable solar hydrogen. The apparent quantum yield for this reaction has been improved, but the lifespan of photocatalysts functioning under sunlight at ambient pressure have rarely been examined, despite the critical importance of this factor in practical applications. Herein, we show that Al-doped SrTiO3 (SrTiO3:Al) loaded with a RhCrO x (rhodium chromium oxide) cocatalyst splits water with an apparent quantum yield greater than 50% at 365 nm. Moreover, following the photodeposition of CoOOH and TiO2, this material maintains 80% of its initial activity and a solar-to-hydrogen energy conversion efficiency greater than or equal to 0.3% over a span of 1300 h under constant illumination by simulated sunlight at ambient pressure. This result is attributed to reduced dissolution of Cr in the cocatalyst following the oxidative photodeposition of CoOOH. The photodeposition of TiO2 further improves the durability of this photocatalyst. This work demonstrates a concept that could allow the design of long-term, large-scale photocatalyst systems for practical sunlight-driven water splitting.Entities:
Year: 2019 PMID: 30996901 PMCID: PMC6430014 DOI: 10.1039/c8sc05757e
Source DB: PubMed Journal: Chem Sci ISSN: 2041-6520 Impact factor: 9.825
Fig. 1Time courses of water-splitting activity of SrTiO3:Al loaded with (a) RhCrO, (b) RhCrO and 0.3 wt% Co species, and (c) RhCrO, 0.3 wt% Co species and 3 wt% TiO2. Reaction conditions: photocatalyst, 0.5 g; reaction solution, 370 mL distilled water; reaction temperature, 291 K; light source, 450 W high-pressure Hg lamp (λ > 300 nm).
Surface atomic ratios of cocatalyst-loaded SrTiO3:Al before and after water splitting reactions under irradiation by a high-pressure Hg lamp (λ > 300 nm)
| Cocatalyst | Reaction time/h | Cr/Ti | Co/Ti |
| RhCrO | 1 | 0.12 | — |
| 168 | 0.07 | — | |
| CoOOH/RhCrO | 0 | 0.21 | 0.27 |
| 168 | 0.20 | 0.25 | |
| TiO2/CoOOH/RhCrO | 0 | 0.06 | 0.04 |
| 168 | 0.06 | 0.04 |
Fig. 2(A) Co-K edge XANES data and (B) Fourier transforms of k3-weighted Co-K EXAFS spectra for (a) CoCl2·6H2O, (b) Co3O4, (c) CoOOH, and RhCrO/SrTiO3:Al coloaded with 0.3 wt% Co species (d) in darkness and (e) following UV illumination for 15 h by a 300 W Xe lamp.
Fig. 3Illustrations of (a) RhCrO/SrTiO3:Al deactivation mechanism and (b) stabilisation of RhCrO/SrTiO3:Al by CoOOH. The stoichiometry of the reactions is ignored for simplicity.
Fig. 4Time course of water splitting activity of 5 × 5 cm2 TiO2/CoOOH/RhCrO/SrTiO3:Al sheet in panel reactor. Reaction conditions: photocatalyst, 20 mg; reaction solution, 1 mm deep distilled water; reaction temperature, 291 K; light source, AM 1.5G solar simulator. Asterisk symbols (*) indicate interruption of the illumination for two days.