2011
DOI: 10.1016/j.crci.2010.11.007
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In situ DRIFTS studies of high-temperature water-gas shift reaction on chromium-free iron oxide catalysts

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Cited by 33 publications
(25 citation statements)
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References 24 publications
(36 reference statements)
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“…It is noteworthy that the peak intensity of this formate species is much higher than that of the carbonate species. Yet, another species with corresponding peaks at 3046 and 3140 cm −1 matched well with those of hydroxyl groups, as reported in the literature 50 . It should be noted that no obvious peaks could be detected in the range of 2000–1800 cm −1 for Ni@SiXNS-EtOH, which reveals the essential absence of bridging CO; this is likely because Ni nanoparticles in the catalyst are trapped between sheets of SiXNS, thus decreasing the chance for the bonding of CO molecules to multiple Ni atoms.…”
Section: Resultssupporting
confidence: 87%
“…It is noteworthy that the peak intensity of this formate species is much higher than that of the carbonate species. Yet, another species with corresponding peaks at 3046 and 3140 cm −1 matched well with those of hydroxyl groups, as reported in the literature 50 . It should be noted that no obvious peaks could be detected in the range of 2000–1800 cm −1 for Ni@SiXNS-EtOH, which reveals the essential absence of bridging CO; this is likely because Ni nanoparticles in the catalyst are trapped between sheets of SiXNS, thus decreasing the chance for the bonding of CO molecules to multiple Ni atoms.…”
Section: Resultssupporting
confidence: 87%
“…38,55 The complex absorption in the 2800-2400 cm -1 region is probably due to a Fermi resonance of the overtone of the OHδ vibration mode with the CHstretching modes at 2971, 2929, and 2863 cm -1 (CH 3 (as), CH 2 (as) and CH 3 (s) modes of the ethoxide species Some remarkable differences between the DRIFTS spectra of samples are observed when the temperature is increased ( Figure 6); acetate bands appear (at 1334, 1439, 1590 cm −1 for the CH3 δ, (OCOν(s), and OCOν(as) vibrations, respectively). 60 The DRIFT spectra obtained on Mn 0.6 Fe 2.4 O 4 (Fig 6-D), also exhibit the bands for acetate species, formed by the reaction of ethoxy species with surface oxygen (1598, 1555, 1433 and 1334 cm -1 ). 59 These species could further produce CO 2 , which is detected as the doublet at the 2358-2338 cm -1 region and corresponds to adsorbed and/or gaseous CO 2 rotation vibration P and R bands.…”
Section: Surface Characterization: Drift Spectroscopymentioning
confidence: 81%
“…By choosing MgO, TiO 2 , and SiO 2 to support iron oxide in this section, it was expected that the large variety of acid-base strengths of MgO (basic support), TiO 2 (amphiprotic support), or SiO 2 (acidic support) important in determining catalytic activity could be realized. In a previous work [12], we have shown that the most active system is the catalyst containing MgO as a support. Fe 2 O 3 /MgO is 12 times more active than Fe 2 O 3 /TiO 2 , 21 times more active than the unsupported catalyst, and 100 times more active than Fe…”
Section: Fe-mg Systemsmentioning
confidence: 95%
“…Boudjemaa et al [3] have reported that magnesium could be a good candidate to replace chromium in iron-based catalysts since Mg-rich catalysts are more active than Cr-promoted ones. By adding MgO to Fe 2 O 3 [12], it was found that the Fe 2 O 3 -MgO basic catalyst is 100 times more active than the acidic catalyst Fe 2 O 3 /SiO 2 and a direct relation between catalytic activity and acid-base properties of catalysts is established.…”
Section: Journal Of Catalystsmentioning
confidence: 99%