1998
DOI: 10.1016/s0022-3115(97)00280-8
|View full text |Cite
|
Sign up to set email alerts
|

Temperature and fission rate effects on the rim structure formation in a UO2 fuel with a burnup of 7.9% FIMA

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

2
17
0

Year Published

2004
2004
2020
2020

Publication Types

Select...
4
4

Relationship

0
8

Authors

Journals

citations
Cited by 33 publications
(19 citation statements)
references
References 14 publications
2
17
0
Order By: Relevance
“…J.Nakamura shows that the crystallites size saturates around 200nm for local burn-up higher than 67 GWd/MtU (pellet average burn-up is 57 GWd/MtU). This is consistent with the value of 300 nm reported by M.Kinoshita [46].…”
Section: A Transformation At Quasi-constant Volumesupporting
confidence: 93%
See 2 more Smart Citations
“…J.Nakamura shows that the crystallites size saturates around 200nm for local burn-up higher than 67 GWd/MtU (pellet average burn-up is 57 GWd/MtU). This is consistent with the value of 300 nm reported by M.Kinoshita [46].…”
Section: A Transformation At Quasi-constant Volumesupporting
confidence: 93%
“…Concerning the temperature threshold for rim formation [46] confirms a value of 1100°C. The limit of the restructured zone was found to be related to the starting of the high fission gas release zone.…”
Section: Burn-up and Temperature Threshold (Local Values)mentioning
confidence: 65%
See 1 more Smart Citation
“…It is well known that UO 2 is exposed to high temperature and irradiation. Such conditions vary widely with position in the fuel, e.g., temperature gradient, high burn-up at the rim region [1], and also vary with loading time, e.g., accumulation of fission products and increase of oxygen partial pressure. As a result, the melting point of uranium oxide is affected by these factors.…”
Section: Introductionmentioning
confidence: 99%
“…For example, several conflicting explanations have been put forward to account for evidence that xenon depletion, pore formation, and recrystallization begin at different local burnups [16]. In addition, a consensus has not been reached on the fission rate and temperature dependence of recrystallization [2,17], on the role of composition and fabrication parameters such as grain size [18], or on the role of stress [19]. This paper, presents a model for irradiation-induced recrystallization that links the observed microstructural evolution of the fuel, the role of fission gas bubbles, and the triggering event for recrystallization.…”
Section: Introductionmentioning
confidence: 99%