Epsilon-phase alloy
precipitates have been observed with varied
compositions and sizes in spent nuclear fuels, such as UO2. The presence of the inclusions, along with other oxide precipitates,
gas bubbles, and irradiation-induced structural defects, can significantly
degrade the physical properties of the fuel. To predict fuel performance,
a fundamental study of the precipitation processes is needed. This
study uses ceria (CeO2) as a surrogate for UO2. Polycrystalline CeO2 films doped with Mo, Ru, Rh, Pd,
and Re (surrogate for Tc) were grown at 823 K using pulsed laser deposition,
irradiated at 673 K with He+ ions, and subsequently annealed
at higher temperatures. A number of methods, including transmission
electron microscopy and atom probe tomography, were applied to characterize
the samples. The results indicate that there is a uniform distribution
of the doped metals in the as-grown CeO2 film. Pd particles
of ∼3 nm in size appear near the dislocation edges after He+ ion irradiation to ∼13 dpa. Thermal annealing at 1073
K in air leads to formation of precipitates of Mo and Pd near the
grain boundaries. Further annealing at 1373 K produces 70 nm sized
precipitates consisting of nanograins at cavities.