Abstract
Hydrogen is a potential alternate energy source for satisfying many of our energy needs. In this work, we studied H2 production from the water-gas-shift (WGS) reaction over Ce1-xCuxO2 catalysts, prepared with a novel microemulsion method, using two synchrotron-based techniques: time-resolved X-ray diffraction (XRD) and X-ray absorption fine structure (XAFS). The results are compared with those reported for conventional CuOx/CeO2 and AuOx/CeO 2 catalysts obtained through impregnation of ceria. For the fresh Ce1-xCuxO2 catalysts, the results of XAFS measurements at the Cu K-edge indicate that Cu is in an oxidation state higher than in CuO. Nevertheless, under WGS reaction conditions the Ce 1-xCuxO2 catalysts undergo reduction and the active phase contains very small particles of metallic Cu and CeO2-x. Time-resolved XRD and XAFS results also indicate that Cuδ+ and Auδ+ species present in fresh CuOx/CeO2 and AuOx/CeO2 catalysts do not survive above 200 °C under the WGS conditions. In all these systems, the ceria lattice displayed a significant increase after exposure to CO and a decrease in H2O, indicating that CO reduced ceria while H2O oxidized it. Our data suggest that H2O dissociation occurred on the Ovacancy sites or the Cu-Ovacancy and Au-Ovacancy interfaces. The rate of H2 generation by a Ce0.95Cu0.05O 2 catalyst was comparable to that of a 5 wt% CuOx/CeO 2 catalyst and much bigger than those of pure ceria or CuO.
Original language | English (US) |
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Pages (from-to) | 81-88 |
Number of pages | 8 |
Journal | Topics in Catalysis |
Volume | 49 |
Issue number | 1-2 |
DOIs | |
State | Published - Jul 2008 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Catalysis
- General Chemistry
Keywords
- Ceria catalysts
- Copper catalysts
- Gold catalysts
- Hydrogen
- In situ characterization
- Water-gas shift reaction
- X-ray absorption fine structure
- X-ray diffraction