2007
DOI: 10.1016/j.chemphys.2007.08.026
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Calculation of X-ray absorption near edge structure of CeO2 using a model cluster

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Cited by 4 publications
(3 citation statements)
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“…Spectra obtained for both the Ce 4+ and Ce 3+ standards were in excellent agreement with previously reported data, displaying a characteristic double peak associated with 4f 1 5d and 4f 0 5d states for Ce 4+ and one single peak for the Ce 3+ corresponding with transitions to unoccupied 4f5d states [17][18][19][20]. Typical spectra recorded from the CeNbO 4.08 and CeNbO 4.25 compositions under ambient conditions (static air and room temperature) are shown in Fig.…”
Section: Resultssupporting
confidence: 80%
“…Spectra obtained for both the Ce 4+ and Ce 3+ standards were in excellent agreement with previously reported data, displaying a characteristic double peak associated with 4f 1 5d and 4f 0 5d states for Ce 4+ and one single peak for the Ce 3+ corresponding with transitions to unoccupied 4f5d states [17][18][19][20]. Typical spectra recorded from the CeNbO 4.08 and CeNbO 4.25 compositions under ambient conditions (static air and room temperature) are shown in Fig.…”
Section: Resultssupporting
confidence: 80%
“…To confirm the presence of Ce(III) centers, two representative samples decomposed at 523 K were studied by means of X-ray absorption near-edge structure (XANES) spectroscopy. Figure shows the Ce L III -edge of pure reference ceria, CL0, and CL20 samples, annealed at 523 K. The characteristic peaks, A and B, and the shoulders, C and D, reported by Suzuki et al for pure CeO 2 are present in both samples, the intensity of A and B being larger in CL0 and CL20, as previously reported for other nanotextured ceria . Both XANES difference spectra (also shown in the inset) present a weak signal at 5724 eV, which reveals a minor fraction of Ce(III) (as compared to Ce(NO 3 ) 3 spectra).…”
Section: Resultssupporting
confidence: 74%
“…However, many calculations about XANES or EELS with the DV‐Xα method were K‐edge or shallow L II, III edge, because the spin‐orbital split due to the relativistic effect need not be considered for these spectra. On the other hand, the relativistic DV‐Xα methods were developed and applied to f‐electron oxides 14, 15. In addition, the multiplet structure was calculated on the basis of these methods 16–21.…”
Section: Introductionmentioning
confidence: 99%