1998
DOI: 10.1016/s0022-3115(97)00280-8
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Temperature and fission rate effects on the rim structure formation in a UO2 fuel with a burnup of 7.9% FIMA

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Cited by 32 publications
(19 citation statements)
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“…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%
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“…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%
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“…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%