Abstract
This report details the continued investigation of process variables involved in converting sol-gel-derived, urania-carbon microspheres to ∼820-μm-dia. UC1-xNx fuel kernels in flow-through, vertical Mo and W crucibles at temperatures up to 2123 K. Experiments included calcining of air-dried UO3-H2O-C microspheres in Ar and H2-containing gases, conversion of the resulting UO2-C kernels to dense UO2:2UC in the same gases and vacuum, and its conversion in N2 to UC1-xNx (x = ∼0.85). The thermodynamics of the relevant reactions were applied extensively to interpret and control the process variables. Producing the precursor UO2:2UC kernel of ∼96% theoretical density was required, but its subsequent conversion to UC1-xNx at 2123 K was not accompanied by sintering and resulted in ∼83–86% of theoretical density. Increasing the UC1-xNx kernel nitride component to ∼0.98 in flowing N2-H2 mixtures to evolve HCN was shown to be quantitatively consistent with present and past experiments and the only useful application of H2 in the entire process.
Original language | English |
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Pages (from-to) | 176-191 |
Number of pages | 16 |
Journal | Journal of Nuclear Materials |
Volume | 483 |
DOIs | |
State | Published - Jan 1 2017 |
Funding
The authors wish to acknowledge the aid and technical insight of K. Terrani, L. Snead and T. Besmann as well as the reviews by G. Helmreich and B. Spencer at ORNL. This paper was supported by the Advanced Fuels Campaign of the Fuel Cycle R&D program in the Office of Nuclear Energy, US Department of Energy.
Funders | Funder number |
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US Department of Energy | |
Office of Nuclear Energy |