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Hydrogen production by tailoring the brookite and Cu 2 O ratio of sol-gel Cu-TiO 2 photocatalysts.

Authors :
Hinojosa-Reyes M
Camposeco-Solís R
Zanella R
Rodríguez González V
Source :
Chemosphere [Chemosphere] 2017 Oct; Vol. 184, pp. 992-1002. Date of Electronic Publication: 2017 Jun 18.
Publication Year :
2017

Abstract

Cu-TiO <subscript>2</subscript> photocatalysts were prepared by the sol-gel method. Copper loadings from, 1.0 to 5.0 wt % were used. The materials were annealed at different temperatures (from 400 to 600 °C) to study the formation of brookite and copper ionic species. The photocatalysts were characterized by X-ray diffraction, UV-vis, Raman and XPS spectroscopies, H <subscript>2</subscript> -temperature programmed reduction (TPR), N <subscript>2</subscript> physisorption, and SEM-EDS to quantify the actual copper loadings and characterize morphology. The photocatalysts were evaluated during the hydrogen photocatalytic production using an ethanolic solution (50% v/v) under UV and visible radiation. The best hydrogen production was performed by Ti-Cu 1.0 with an overall hydrogen production that was five times higher than that obtained with photolysis. This sample had an optimal thermal treatment at 500 °C, and at this temperature, the Cu <subscript>2</subscript> O and brookite/anatase ratio boosted the photocatalytic production of hydrogen. In addition, a deactivation test was carried out for the most active sample (TiO <subscript>2</subscript> -Cu 1.0), showing unchanged H <subscript>2</subscript> production for three cycles with negligible Cu lixiviation. The activity of hydrogen-through-copper production reported in this research work is comparable with the one featured by noble metals and that reported in the literature for doped TiO <subscript>2</subscript> materials.<br /> (Copyright © 2017 Elsevier Ltd. All rights reserved.)

Details

Language :
English
ISSN :
1879-1298
Volume :
184
Database :
MEDLINE
Journal :
Chemosphere
Publication Type :
Academic Journal
Accession number :
28658742
Full Text :
https://doi.org/10.1016/j.chemosphere.2017.06.066