Abstract
Co3O4 is a promising catalyst for removing CO from H2 streams via the preferential CO oxidation (PROX). A Mars-van-Krevelen redox mechanism is often suggested but a detailed knowledge especially of the oxidation state of the catalytically active surface under reaction conditions is typically missing. We have thus utilized operando X-ray absorption spectroscopy to examine structure and oxidation state during PROX, and near atmospheric pressure-XPS at low photoelectron kinetic energies and thus high surface sensitivity to monitor surface composition changes. The rather easy surface reduction in pure CO (starting already at ∼100 °C) and the easy reoxidation by O2 suggest that molecularly adsorbed CO reacts with lattice oxygen, which is replenished by gas phase O2. Nevertheless, the steady state concentration of oxygen vacancies under reaction conditions is too low even for XPS detection so that both the bulk and surface of Co3O4 appear fully oxidized during PROX. Furthermore, the effect of adding CeO2 (a less active material) to Co3O4 was studied. Promotion of Co3O4 with 10 wt% CeO2 increases the reduction temperatures in CO and H2 and enhances the PROX activity. Since CeO2 is a less active material, this can only be explained by a higher activity of the Co-O-Ce interface.
| Originalsprache | Englisch |
|---|---|
| Seitenumfang | 15 |
| Fachzeitschrift | Journal of catalysis |
| Jahrgang | 344.2016 |
| Ausgabenummer | December |
| DOIs | |
| Publikationsstatus | Elektronische Veröffentlichung vor Drucklegung. - 23 Sept. 2016 |
| Extern publiziert | Ja |
Bibliographische Notiz
Funding Information:This work was supported by the Austrian Science Fund (FWF) in the framework of the Doctoral School “Building Solids for Function (“Solids4Fun”) [project W1243] and by project “Cobalt Oxide Model Catalysis” (“ComCat”) [I 1041-N28]. We acknowledge the Helmholtz-Zentrum Berlin for synchrotron radiation beamtime at ISISS beamline of BESSY II and the beamtime granted at the I811 beamline at the MAX-lab synchrotron radiation source, Lund University, Sweden, and support by Dr. Stefan Carlson. The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 312284. We are grateful to Dr. Klaudia Hradil and DI Werner Artner for assistance with the XRD measurements.
Publisher Copyright:
© 2016 The Author(s)
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