1998
DOI: 10.1023/a:1019098121432
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Cited by 74 publications
(47 citation statements)
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“…4 shows the DRIFT spectra of CO 2 and CO adsorbed on 1 wt.% Pt/CeO 2 . When CO 2 is exposed to Pt/CeO 2 on the DRIFT Procedure B, the absorption peaks assigned to the hydrogenocarbonate species were observed at around 1630, 1350 and 1060 cm À1 [20][21][22], and the absorption peaks assigned to the monodentate carbonate species were observed at 1520 and 1270 cm À1 [21][22][23][24]. The intensities of these peaks were much higher than those observed for the CO adsorption treatment in Fig.…”
Section: Evaluation Of Precious Metal Dispersions On Ceo 2 -Zromentioning
confidence: 73%
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“…4 shows the DRIFT spectra of CO 2 and CO adsorbed on 1 wt.% Pt/CeO 2 . When CO 2 is exposed to Pt/CeO 2 on the DRIFT Procedure B, the absorption peaks assigned to the hydrogenocarbonate species were observed at around 1630, 1350 and 1060 cm À1 [20][21][22], and the absorption peaks assigned to the monodentate carbonate species were observed at 1520 and 1270 cm À1 [21][22][23][24]. The intensities of these peaks were much higher than those observed for the CO adsorption treatment in Fig.…”
Section: Evaluation Of Precious Metal Dispersions On Ceo 2 -Zromentioning
confidence: 73%
“…Moreover, the other peaks assigned to the hydrogenocarbonate species appeared at ca. 1630 and 1270 cm À1 [20][21][22], and the peak assigned to the monodentate carbonate species appeared at ca. 1520 cm À1 [21][22][23][24].…”
Section: Evaluation Of Precious Metal Dispersions On Ceo 2 -Zromentioning
confidence: 99%
See 1 more Smart Citation
“…These studies have also observed the presence of surface-bound formate species under reaction conditions [16] and also have measured the stability of these species in inert gas and hydrogen [17,18]. Compared with single crystal copper surfaces, the surface species observed on the oxide supported polycrystalline copper system are more complex because of the multi-faceted copper surfaces presented by the supported particles [14,17,[19][20][21] and the presence of species adsorbed on the support materials (e.g., alumina and ceria) as well as the support-metal interface [22]. More complex infrared spectra are observed which makes assignment more difficult than on the single crystals [23][24][25].…”
Section: Introductionmentioning
confidence: 99%
“…The presence of vacancies in rods and cubes is supported by the FTIR spectra in helium ( Figure 24) showing that the integrated intensity ratio of carbonates to OH groups in rods and cubes is significantly higher compared to that in octahedra. The formation of carbonates on ceria is due to the interaction with CO 2 from the ambient, resulting in the reduction of ceria to Ce 3+ and hence the creation of oxygen vacancies [141][142][143].…”
Section: Discussionmentioning
confidence: 99%