264926 Effect of Iron and Titanium Oxide Promoters On Platinum Model Catalysts for the Water-Gas Shift Reaction

Monday, October 29, 2012: 4:15 PM
321 (Convention Center )
M. Cem Akatay1, Jorge Pazmino2, Mayank Shekhar2, W. Damion Williams2, Anil Mane3, Eric A. Stach4, W. Nicholas Delgass2, Jeffrey W. Elam5, Dmitry Zemlyanov6 and Fabio H. Ribeiro2, (1)School of Materials Engineering and Birck Nanotechnology Center, Purdue University, West Lafayette, IN, (2)School of Chemical Engineering, Purdue University, West Lafayette, IN, (3)Argonne National Laboratory, Argonne, IL, (4)Center for Functional Nanomaterials, Brookhaven National Laboratory, Upton, NY, (5)Energy Systems Division, Argonne National Laboratory, Lement, IL, (6)Birck NanoTechnology Center, Purdue University, West Lafayette, IN

Iron oxide and titania enhance the water-gas shift (WGS) reaction rate per surface area of metal on palladium and platinum catalysts. To study the effect of these promoters, we prepared samples on ceria and non-porous model spherical alumina supports by atomic layer deposition. Employing promoters deposited as monolayers (as opposed to studying the promoter as a bulk support) is advantageous as the signal from the promoter can come only from the surface.

One set of samples is 3.6 wt% Pt/Al2O3 sample promoted with 10 wt% TiO2 and another 0.5 wt% Pt/Al2O3 promoted with 11 wt% Fe. The WGS reaction rate for the titania promoted sample is 1.3×10-2 and that for Fe promoted sample is 4.5×10-2 mole H2 mole Pt-1 s-1 under 7% CO, 8.5% CO2, 22% H2O, 37% H2 at 1 atm total pressure at 250 oC, a promotion of a factor of 17 and 60, respectively when compared with the un-promoted Pt/Al2O3 catalyst.

The catalysts were analyzed in situ under 0.5 mbar pressure using ambient pressure synchrotron-based Photoemission Spectroscopy (PES). High-resolution core-level spectra were obtained both under reducing atmosphere of H2 at 300 oC and under the WGS reaction mixture of 7% CO, 2% H2O, 37% H2, 9% CO2 at 250 oC at a total pressure of 0.5 mbar. The probed volume depends on the escape depth of photoelectrons, which is a function of photoelectron kinetic energy. To obtain the depth profile, the photon energy of the exciting radiation was varied so as to obtain the kinetic energy of photoelectrons ranging from 120 to 420 eV. The oxidation state of metals under different atmospheres and change in composition as a function of depth were investigated. Based on the findings, models describing the structure of catalysts were developed and compared to images obtained by Environmental High-Resolution Transmission Electron Microscopy (HR-TEM).

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