Avgouropoulos, G.

Boccuzzi, F.

Idakiev, V.

Ioannides, T.

Manzoli, M.

Papavasiliou, J.

Tabakova, T.

Tenchev, K.

English

Manzoli, Maela

Boccuzzi, Flora

Institutional Research Information System University of Turin

Impact of the support composition on the performance of  Au/CeO2-Fe2O3 catalysts in PROX and WGS reactions   T. Tabakova a,*, G. Avgouropoulos b, J. Papavasiliou b, M. Manzoli c, F. Boccuzzi c, V. Idakiev a, K. Tenchev a, T. Ioannides b  a Institute of Catalysis, Bulgarian Academy of Sciences, Sofia 1113, Bulgaria, E-mail: tabakova@ic.bas.bg  b Foundation for Research and Technology-Hellas (FORTH), Institute of Chemical Engineering and High-Temperature Chemical Processes (ICE-HT), Patras GR-265 00, Greece c Department of Chemistry IFM and NIS Centre of Excellence, University of Torino, Torino 10125, Italy  Introduction   The utilization of pure hydrogen as energy source in proton exchange membrane fuel cells has stimulated extensive research for development of active WGS and PROX catalysts. Au/ceria catalysts have been proven very efficient for both reactions [1,2]. The stability of catalysts under operating conditions is an important issue. A very recent study of Au/doped-ceria catalysts for PROX has revealed the beneficial role of ceria modification for activity enhancement and improved resistance towards deactivation caused by the presence of CO2 and H2O in the PROX feed [3]. Mixed CeO2-Fe2O3 oxides with different ratio were prepared and used as supports of gold catalysts in order to optimize their performance. The selection of these oxides was based on previous experience and on the following considerations: i) Fe2O3 is the main component of high-temperature WGS catalysts. Investigations of Au/Fe2O3 catalysts have shown that it is also a very suitable support for active low-temperature WGS and PROX catalysts [4,5]; ii) ceria is interesting because of its unique redox properties, high oxygen storage capacity and ability to promote metal dispersion.   Experimental   CeO2-Fe2O3 oxides with atomic ratio Ce/(Ce+Fe) 0.25, 0.50 and 0.75, (as well as pure CeO2 and Fe2O3) were synthesized by coprecipitation using urea as precipitation agent. The gold catalysts (3.5 wt.% Au) were prepared by the deposition-precipitation method and characterized by N2 physisorption, XRD, HRTEM, FTIR and H2-TPR. The catalytic activity and selectivity measurements for PROX and WGS reactions were carried out `in conventional flow reactor systems [3,4].  Results and discussion  XRD diffraction peaks related to fluorite structure of CeO2, hematite structure of α-Fe2O3 and metallic Au are easy detectable in the XRD patterns of the catalysts. The intensity of the peaks of CeO2 continuously weakens, while those of hematite intensify with the increase of Fe2O3 content. The intensity of Au0 main peak is minimized for AuCe0.5Fe0.5. The analysis of TPR profiles reveals a significant effect of gold on the reducibility of mixed oxides. The peaks, which are related to the surface reduction of ceria and of hematite-to-magnetite in TPR profiles of mixed oxide catalysts shift to lower temperatures. The surface ceria reduction in Au/Ce0.5Fe0.5 occurs at lower temperature (130 oC) than in Au/Ce0.75Fe0.25, which has a higher CeO2 content (150 oC). This result correlates with the observed catalytic activity-selectivity trends in the PROX reaction (Fig. 1). Moreover, Au/Ce0.5Fe0.5 exhibits the best tolerance to the presence of CO2 and H2O in the feed. FTIR spectra collected after CO+O2 interaction at 90 K evidence better reactivity of Au/Ce0.5Fe0.5 compared to Au/Ce0.75Fe0.25, as confirmed by the strong intensity of the band at 2341 cm-1 due to CO2 produced in the presence of a high concentration of metallic Au particles (band at 2102 cm-1) on the surface of this catalyst. WGS activity tests demonstrate also better performance of Au/Ce0.5Fe0.5 in comparison with Au/Ce0.75Fe0.25. Figure 1. Catalytic behavior of Au/CeO2-Fe2O3 catalysts in CO PROX reaction.  Figure 2. FTIR absorption spectra after interaction between CO and O2 at 90 K. Conclusions Gold particle size, the nature and the amount of Au sites depend on the composition of mixed CeO2-Fe2O3 oxides. These properties strongly influence the catalytic performance of the supported gold catalysts in PROX and WGS reactions. In order to obtain a better understanding of the behavior of the catalysts, detailed characterization by HRTEM and FTIR spectroscopy will be reported. References [1] Burch, R., Gold catalysts for pure H2 production in the WGSR: activity, structure and reaction mechanism, Physical Chemistry Chemical Physics, 8 (2006), 5483-5500 and references therein. [2] Schubert, M.M., Plzak, V., Garche, J., Behm, R.J., Activity, selectivity, and long-term stability of different metal oxide supported gold catalysts for the CO PROX in H2-rich gas, Catalysis Letters, 76 (2001), 143-150. [3] Avgouropoulos, G., Manzoli, M., Boccuzzi, F., Tabakova, T., Papavasiliou, J., Ioannides, T., Idakiev, V., Catalytic performance and characterization of Au/doped-CeO2 catalysts for the CO PROX reaction, Journal of Catalysis, 256 (2008), 237-247. [4] Andreeva, D., Idakiev, V., Tabakova, T., Andreev, A., Low-temperature WGSR over Au/a-Fe2O3, Journal of Catalysis, 158 (1996), 354-355. [5] Avgouropoulos, G., Ioannides, T., Papadopoulou, Ch., Batista, J., Hocevar, S., Matralis, H., A comparative study of Pt/γ-Al2O3, Au/α-Fe2O3 and CuO–CeO2 catalysts for the selective oxidation of CO in excess hydrogen, Catalysis Today, 75 (2002), 157-167. 

Impact of the support composition on the performance of Au/CeO2-Fe2O3 catalysts in PROX and WGS reactions

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Impact of the support composition on the performance of Au/CeO2-Fe2O3 catalysts in PROX and WGS reactions

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