2006
DOI: 10.1016/j.cattod.2005.11.023
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Structure–reactivity relationships in VO /TiO2 catalysts for the oxyhydrative scission of 1-butene and n-butane to acetic acid as examined by in situ-spectroscopic methods and catalytic tests

Abstract: Different VO x /TiO 2 catalyst have been catalytically tested and studied by in situ-spectroscopic methods (FT-IR, UV/vis, EPR) in the oxyhydrative scission (OHS) of 1-butene and n-butane to acetic acid (AcOH). While 1-butene OHS follows the sequence butane → butoxide → ketone → AcOH/acetate with a multitude of side products also formed, n-butane OHS leads to AcOH, CO x and H 2 O only. Water vapour in the feed improves AcOH selectivity by blocking adsorption sites for acetate. The admixture of Sb 2 O 3 was fou… Show more

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Cited by 10 publications
(2 citation statements)
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References 13 publications
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“…For comparative purposes, the spectrum of the catalyst reduced in H 2 (see Section 2.3) is also shown in this figure. An increase in the relative Kubelka-Munk function in the 420-800 nm range after 0.5 h in H 2 flow at 823 K is related to the reduction of V 5+ to V 4+ /V 3+ [28,38,39]. From this UV/Vis spectrum and our findings made in the in situ spectroscopic study of VO x /SiO 2 -TiO 2 redox behavior [39], we conclude that the changes in the UV/Vis spectra of VO x /MCM-41 during DH reaction are related to the formation of coke species.…”
Section: Analysis Of Formation and Removal Of Carbon Depositsmentioning
confidence: 95%
“…For comparative purposes, the spectrum of the catalyst reduced in H 2 (see Section 2.3) is also shown in this figure. An increase in the relative Kubelka-Munk function in the 420-800 nm range after 0.5 h in H 2 flow at 823 K is related to the reduction of V 5+ to V 4+ /V 3+ [28,38,39]. From this UV/Vis spectrum and our findings made in the in situ spectroscopic study of VO x /SiO 2 -TiO 2 redox behavior [39], we conclude that the changes in the UV/Vis spectra of VO x /MCM-41 during DH reaction are related to the formation of coke species.…”
Section: Analysis Of Formation and Removal Of Carbon Depositsmentioning
confidence: 95%
“…It can be seen that the ultraviolet absorption edge wavelength of MIL‐88B(V) was 490 nm, which was 15 nm higher than the 475 nm ultraviolet absorption edge wavelength of MIL‐101(V). Generally, the greater the ultraviolet absorption wavelength, the higher the degree of polymerization of the V species [35,43–44] . It can be inferred from the solid ultraviolet diffuse reflection results that the V species in MIL‐88B(V) had higher degree of polymerization and more V−O−V bonds, which may provide more acid sites in the SCR reaction.…”
Section: Resultsmentioning
confidence: 99%