Apr 9, 2025
3:30pm - 4:00pm
Summit, Level 3, Room 339
Larry Aagesen1,2,Sudipta Biswas1,Pierre-Clement Simon1,Kyle Gamble1,Michael Cooper3,Conor Galvin3,David Andersson3,Sophie Blondel4,Wen Jiang5
Idaho National Laboratory1,University of Michigan–Ann Arbor2,Los Alamos National Laboratory3,The University of Tennessee, Knoxville4,North Carolina State University5
Larry Aagesen1,2,Sudipta Biswas1,Pierre-Clement Simon1,Kyle Gamble1,Michael Cooper3,Conor Galvin3,David Andersson3,Sophie Blondel4,Wen Jiang5
Idaho National Laboratory1,University of Michigan–Ann Arbor2,Los Alamos National Laboratory3,The University of Tennessee, Knoxville4,North Carolina State University5
To improve the economics of light water reactors for commercial nuclear energy generation, utility operators are seeking to obtain regulatory approval to run UO2 fuel to higher levels of burnup. One potential impediment to obtaining this approval is the phenomenon of fuel fragmentation, relocation, and dispersal (FFRD). FFRD can result when fuel experiences a rapid temperature transient, such as that occurring during a Loss Of Coolant Accident (LOCA). FFRD has historically been most associated with the rim region in UO2 fuel pellets, where the phenomenon of fragmentation is also referred to as pulverization due to the small size of the fragments. More recent evidence suggests that the so-called “dark zone” (due to its appearance in micrographs) that can be observed in the mid-radial regions of high burnup fuel is also susceptible to FFRD. Although empirical fuel performance models have been developed that can adequately predict pulverization in the rim region under typical LWR conditions, a scientific understanding of what underlies fuel restructuring and subsequent FFRD is lacking even in the rim region, and no models are currently available for the behavior the dark zone. To address these challenges, the U.S. Department of Energy’s Nuclear Energy Advanced Modeling and Simulation (NEAMS) program has employed a multi-scale modeling approach to improve scientific understanding and develop new fuel performance models. In this talk, I will focus on meso-scale efforts, which form a crucial link between atomic-scale and engineering-scale models. Phase-field modeling combined with cluster dynamics is used to predict the restructuring process in the rim region. Phase-field fracture modeling, informed by atomistic simulations, is used to predict the onset of pulverization in the rim region. Combining these techniques together allows the extent of rim pulverization to be predicted. The formation and evolution of the dark zone has also been simulated with the phase-field method, using an improved approach to vacancy source term parameterization. The work shows the important impact of microstructure on fuel performance.