Chromium and copper doubly promoted ceria catalysts have been prepared by three routes: (i) coprecipitation from aqueous solutions containing cerium(IV), copper(II), and chromium(III) ions, (ii) sequential impregnation of CeO 2 by using an aqueous CrO 3 solution followed by an aqueous solution of copper(II) nitrate, and (iii) impregnation of Cu(II)/CeO 2 prepared by coprecipitation by using an aqueous CrO 3 solution. The nature of the chemical transformations occurring during the thermal processing of the catalyst materials obtained by route (i) have been investigated by a combination of FT-IR, powder X-ray diffraction, transmission electron microscopy, X-ray absorption spectroscopy, and electron paramagnetic resonance spectroscopy. Some comparative data for materials obtained by the other two routes is also described. The nature of the transition-metal promoters varies substantially with the calcination processing temperature, the preparative route, and the Cu/Cr content. At low processing temperatures, copper is present as Cu(OH) 2 (polymeric) in the Cu/Cr/CeO 2 -cop material, but a variety of chromium species in oxidation states +III, +V, and +VI are observed. After thermal processing at 573 K, the material comprises small crystallites of ceria-supporting amorphous copper(II) and chromium(III), chromium(V), and chromium(VI) oxide species. Significant physical and chemical changes occur to the material by 873 K, which comprises crystallites of CeO 2 and the spinel CuCr 2 O 4 which is converted at 1273 K to Cu 2 Cr 2 O 4, although a crystalline Cr 2 O 3 phase separates with high chromium loadings. Chromium is present as adsorbed {Cr 2 O 7 2 - } ions in the Cu/Cr/CeO 2 -imp/imp and Cu/Cr/CeO 2 -cop/imp materials at low-thermal treatments, but the dimeric surface anion is largely decomposed at 573 K although chromium(VI) is still present in substantial quantities. No ternary oxide phases are formed in either of these materials on thermal processing at high temperatures, and only phase-separated Cr 2 O 3 and CuO are formed at temperatures from 873 to 1273 K.
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Harrison et al. (2002) studied this question.
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