Abstract
Self-supported films of CeO1.95 display time-scale dependent elastic moduli, a phenomenon which has been termed the chemical strain effect. In order to probe the possible structural origins of this behavior, extended X-ray absorption fine structure spectroscopy and X-ray diffraction were used. Evidence was found that, although this oxygen deficient ceria appears to maintain the fluorite structure on average, the mean Ce-O bond length is shorter than the mean Ce-oxygen vacancy distance. This finding is consistent with crystallographic data from more strongly reduced ceria in which the oxygen vacancies are ordered. By studying strain induced structural changes, we show that it is possible to relate this lattice distortion to the chemical strain effect. Similar conclusions were previously reached for films of Ce 0.8Gd0.2O1.9. Since the ionic radii of both Gd3+ and Ce3+ are larger than that of Ce4+, we suggest that when cation dopants are larger than the host, ceria compounds containing a high concentration of oxygen vacancies may exhibit elastic anomalies.
| Original language | English |
|---|---|
| Pages (from-to) | 1473-1477 |
| Number of pages | 5 |
| Journal | Solid State Ionics |
| Volume | 181 |
| Issue number | 33-34 |
| DOIs | |
| Publication status | Published - Oct 25 2010 |
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Keywords
- Chemical strain
- Elasticity
- Extended X-ray absorption fine structure spectroscopy (EXAFS)
- Gadolinium-doped ceria
- Thermal expansion
ASJC Scopus subject areas
- Materials Science(all)
- Condensed Matter Physics
- Chemistry(all)
Cite this
The origin of elastic anomalies in thin films of oxygen deficient ceria, CeO2 - X . / Kossoy, Anna; Frenkel, Anatoly I.; Feldman, Yishay; Wachtel, Ellen; Milner, Alla; Lubomirsky, Igor.
In: Solid State Ionics, Vol. 181, No. 33-34, 25.10.2010, p. 1473-1477.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - The origin of elastic anomalies in thin films of oxygen deficient ceria, CeO2 - X
AU - Kossoy, Anna
AU - Frenkel, Anatoly I.
AU - Feldman, Yishay
AU - Wachtel, Ellen
AU - Milner, Alla
AU - Lubomirsky, Igor
PY - 2010/10/25
Y1 - 2010/10/25
N2 - Self-supported films of CeO1.95 display time-scale dependent elastic moduli, a phenomenon which has been termed the chemical strain effect. In order to probe the possible structural origins of this behavior, extended X-ray absorption fine structure spectroscopy and X-ray diffraction were used. Evidence was found that, although this oxygen deficient ceria appears to maintain the fluorite structure on average, the mean Ce-O bond length is shorter than the mean Ce-oxygen vacancy distance. This finding is consistent with crystallographic data from more strongly reduced ceria in which the oxygen vacancies are ordered. By studying strain induced structural changes, we show that it is possible to relate this lattice distortion to the chemical strain effect. Similar conclusions were previously reached for films of Ce 0.8Gd0.2O1.9. Since the ionic radii of both Gd3+ and Ce3+ are larger than that of Ce4+, we suggest that when cation dopants are larger than the host, ceria compounds containing a high concentration of oxygen vacancies may exhibit elastic anomalies.
AB - Self-supported films of CeO1.95 display time-scale dependent elastic moduli, a phenomenon which has been termed the chemical strain effect. In order to probe the possible structural origins of this behavior, extended X-ray absorption fine structure spectroscopy and X-ray diffraction were used. Evidence was found that, although this oxygen deficient ceria appears to maintain the fluorite structure on average, the mean Ce-O bond length is shorter than the mean Ce-oxygen vacancy distance. This finding is consistent with crystallographic data from more strongly reduced ceria in which the oxygen vacancies are ordered. By studying strain induced structural changes, we show that it is possible to relate this lattice distortion to the chemical strain effect. Similar conclusions were previously reached for films of Ce 0.8Gd0.2O1.9. Since the ionic radii of both Gd3+ and Ce3+ are larger than that of Ce4+, we suggest that when cation dopants are larger than the host, ceria compounds containing a high concentration of oxygen vacancies may exhibit elastic anomalies.
KW - Chemical strain
KW - Elasticity
KW - Extended X-ray absorption fine structure spectroscopy (EXAFS)
KW - Gadolinium-doped ceria
KW - Thermal expansion
UR - http://www.scopus.com/inward/record.url?scp=77958099002&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77958099002&partnerID=8YFLogxK
U2 - 10.1016/j.ssi.2010.09.001
DO - 10.1016/j.ssi.2010.09.001
M3 - Article
AN - SCOPUS:77958099002
VL - 181
SP - 1473
EP - 1477
JO - Solid State Ionics
JF - Solid State Ionics
SN - 0167-2738
IS - 33-34
ER -