Interplay of defect cluster and the stability of xenon in uranium dioxide by density functional calculations
Hua Y. Geng, Ying Chen, Yasunori Kaneta, Motoyasu Kinoshita, and Q. Wu

TL;DR
This study uses first-principles calculations to explore how defect clusters influence xenon behavior in uranium dioxide, revealing thermodynamic preferences and charge states that impact bubble growth in nuclear fuel.
Contribution
It provides new insights into xenon defect interactions in UO2 under realistic conditions, extending previous models with detailed thermodynamic and charge state analysis.
Findings
Oxygen defect clusters increase xenon solution energy by 0.5 eV.
Xenon prefers tri-vacancy sites in hypo-stoichiometric conditions.
Uranium vacancies are favored for xenon in hyper-stoichiometric regimes.
Abstract
Self-defect clusters in bulk matrix might affect the thermodynamic behavior of fission gases in nuclear fuel such as uranium dioxide. With first-principles LSDA+U calculations and taking xenon as a prototype, we find that the influence of oxygen defect clusters on the thermodynamics of gas atoms is prominent, which increases the solution energy of xenon by a magnitude of 0.5 eV, about 43% of the energy difference between the two lowest lying states at 700 K. Calculation also reveals a thermodynamic competition between the uranium vacancy and tri-vacancy sites to incorporate xenon in hyper-stoichiometric regime at high temperatures. The results show that in hypo-stoichiometric regime neutral tri-vacancy sites are the most favored position for diluted xenon gas, whereas in hyper-stoichiometric condition they prefer to uranium vacancies even after taking oxygen self-defect clusters into…
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