Synchrotron Microdiffraction Study of Heavy-Ion-Irradiated Uranium-Molybdenum Dispersion Fuel
There has been an ongoing effort by the Department of Energy Office of Material Management and Minimization to convert research and test reactors from high-enriched to low-enriched uranium fuels. Uranium-molybdenum alloy fuel dispersed in an aluminum matrix (UMo-Al dispersion fuel) has emerged as the leading candidate fuel for converting the remaining high-power research reactors in Europe. One of the primary barriers to using this fuel type is the deleterious reaction of UMo with Al. Depending on the operating temperature of the reactor, this interaction layer can be amorphous under irradiation and allows for the accumulation of fission gas products in large bubbles, leading to unacceptable swelling of the fuel. Therefore, detailed characterization of the phases that form within the fuel and in the interaction layer is critical to understanding, and controlling, UMo-Al dispersion fuel behavior under irradiation. Furthermore, the phase stability of the UMo fuel is of great importance, as the alpha-UMo phase has undesirable swelling compared to the metastable gamma-UMo phase. Heavy ion irradiation was used to reproduce the interaction layer that develops in-reactor. Samples of both the fuel and interaction layer formed under ion irradiation were examined using the high-energy x-ray microdiffraction technique at the Advanced Photon Source (APS) at Argonne National Laboratory to examine the microstructure of the interaction layer. The high-resolution phase information obtained in this experiment provides a valuable basis for understanding the evolution of UMo-Al dispersion fuel under irradiation and as input for computational studies to improve predictive capabilities. Phase information for in-pile fuels can currently be determined from TEM samples (limited sample volume, limiting statistics), or by extrapolation from SEMEDS analysis. (authors)