Significantly enhanced cocatalyst-free H-2 evolution from defect-engineered Brown TiO2

TiO2 is the extensively investigated materials for various photocatalytic reforming and water splitting. Superior stability towards photo-corrosion, appropriate band energy levels driving most photocatalytic reactions, and lowcost production are promising features of TiO2. However, a primary limitat...

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Veröffentlicht in:Ceramics international 2021-05, Vol.47 (10), p.14821-14828
Hauptverfasser: Babu, S. Jagadees, Rao, V. Navakoteswara, Murthy, Dharmapura H. K., Shastri, Mahesh, Murthy, M., Shetty, Manjunath, Raju, K. S. Anantha, Shivaramu, Prasanna D., Kumar, C. S. Ananda, Shankar, M. V., Rangappa, Dinesh
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Sprache:eng
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Zusammenfassung:TiO2 is the extensively investigated materials for various photocatalytic reforming and water splitting. Superior stability towards photo-corrosion, appropriate band energy levels driving most photocatalytic reactions, and lowcost production are promising features of TiO2. However, a primary limitation with TiO2 is that it only absorbs ultraviolet light constituting less than 5% of the solar spectrum. In this work, we use a facile, low temperature, vacuum-free, and solution-route synthesis approach to rationally induce oxygen vacancy/Ti3+ defects to reduce the bandgap of TiO2 to 2.0 eV (3.2 eV for pristine white TiO2) to form brown TiO2 with enhanced visible-light absorption. The mechanism of defect formation is systematically deduced from the detailed investigation through Raman spectroscopy, spin-sensitive technique, high-resolution microscopy, and surface analysis. The brown TiO2 yielded 8.1 mmol h(-1)g(cat)(-1) H-2 evolution without any cocatalyst under natural sunlight, which is a factor two higher than pristine (white) TiO2. To the best of our knowledge, the observed H-2 evolution rate is the highest reported value under natural sunlight for any TiO2-based photocatalyst. This work demonstrates the applicability of brown TiO2 to fabricate large-area photocatalyst panels for the cost-effective production of solar H-2.
ISSN:0272-8842
1873-3956
DOI:10.1016/j.ceramint.2020.10.026