Abstract
The structure of several nano-sized ceria, CeO2, systems was investigated using neutron and X-ray diffraction and X-ray absorption spectroscopy. Whilst both diffraction and total pair distribution functions (PDFs) revealed that in all of the samples the occupancy of both Ce4+ and O2− are very close to the ideal stoichiometry, the analysis using Reverse Monte Carlo technique revealed significant disorder around oxygen atoms in the nano-sized ceria samples in comparison to the highly crystalline NIST standard. In addition, the analysis revealed that the main differences observed in the pair correlations from various X-ray and neutron diffraction techniques were attributable to the particle size of the CeO2 prepared by the reported three methods. Furthermore, detailed analysis of the Ce L3- and K-edge EXAFS data support this finding; in particular the decrease in higher shell coordination numbers with respect to the NIST standard, is attributed to differences in particle size.
| Original language | English |
|---|---|
| Pages (from-to) | 3494-3503 |
| Number of pages | 10 |
| Journal | ChemPhysChem |
| Volume | 17 |
| Issue number | 21 |
| DOIs | |
| State | Published - Nov 4 2016 |
| Externally published | Yes |
Keywords
- EXAFS
- Reverse Monte Carlo
- Rietveld analysis
- ceria
- pair distribution functions