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dc.contributor.authorHarrison, Philip G.-
dc.contributor.authorThornton, Edward W.-
dc.date.accessioned2025-11-18T10:37:50Z-
dc.date.available2025-11-18T10:37:50Z-
dc.date.issued1978-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/20088-
dc.description.abstractAn experimental study has been carried out on the mechanism of formation of a surface isocyanate species on the mixed oxide catalyst SnO2· 0·55 CuO during the initial stages of catalysis of the CO + NO reaction at ≈470 K. Using infrared spectroscopy, the isotopic shifts of the 2189 cm–1 pseudo-antisymmetric stretching vibration have been measured for 13C, 15N and 18O substitution. The oxygen atom of the surface isocyanate has been shown to originate from NO rather than CO as was previously assumed. This observation has been interpreted in terms of a mechanism involving initial dissociative chemisorption of CO followed by the formation of a fulminate via reaction of NO with the surface carbon atom and subsequent rapid isomerisation to the isocyanate: [graphic omitted].en_US
dc.language.isoenen_US
dc.publisherJournal of the Chemical Society : Faraday Transaction - I. The Chemical Society, London. 1978, 74 (09-12)en_US
dc.subjectChemistryen_US
dc.subjectInfrared spectroscopyen_US
dc.subjectAdsorbate identificationen_US
dc.subjectJournal of the Chemical Society : Faraday Transaction - Ien_US
dc.titleTin oxide surfaces. Part 8.—Infrared study of the mechanism of formation of a surface isocyanate species on SnO2· 0·55 CuO during catalysis of the oxidation of carbon monoxide by nitric oxideen_US
dc.typeArticleen_US
Appears in Collections:Journal Articles (before-1995)

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