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Title: Infrared studies of CO and/or NO adsorption on reduced W/Al sub 2 O sub 3 catalysts

Journal Article · · Journal of Catalysis; (United States)
OSTI ID:5757783

Infrared spectroscopy (IR) has been used to investigate CO and/or NO adsorption on reduced W/Al{sub 2}O{sub 3} catalysts. The effect of reduction temperature and tungsten-loading was studied. Three different kinds of surface W-sites were identified according to the IR spectra (possibly W{sup 5+}, W{sup 4+} (I), and W{sup 4+} (II)). Up to three IR bands at 2,198, 2,176, and 2,154 cm{sup {minus}1} for adsorbed CO, which are best assigned to W{sup 5+} (CO), W{sup 4+} (I) (CO), and W{sup 4+} (II) (CO), respectively, were observed. Only two kinds of surface complexes, W{sup 5+} (NO) with a single band at 1,843 cm{sup {minus}1} and W{sup 4+} (I and II) (NO){sub 2} with coupled bands at 1,780 and 1,691 cm{sup {minus}1}, were formed upon NO contact. In the case of CO + NO and NO + CO (added in sequence) coadsorption, a surface complex in the form of (CO) W{sup 4+} (I) (NO){sub 2}, which gave three IR bands at about 2,117, 1,801, and 1,725 cm{sup {minus}1}, was evidenced in the spectra in addition to W{sup 5+} (CO) and W{sup 4+} (II) (NO){sub 2} on the surface. These observations suggest that W{sup 4+} (I)-sites differ from W{sup 4+} (II)-sites in the coordination state and the coadsorption of CO + NO or NO + CO allows more information about the surface W-sites to be achieved than the corresponding CO or NO single adsorption in IR studies. The adsorption and desorption mechanisms are discussed for the surface complex of (CO) W{sup 4+} (I) (NO){sub 2}. Laser Raman spectroscopy (LRS) and temperature-programmed reduction (TPR) were also employed as complementary techniques to characterize the W/Al{sub 2}O{sub 3} catalysts. The results from these two measurements are in good agreement with the IR results.

OSTI ID:
5757783
Journal Information:
Journal of Catalysis; (United States), Vol. 131:1; ISSN 0021-9517
Country of Publication:
United States
Language:
English

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