Kinetics of precipitation of U4O9 from hyperstoichiometric UO2+x
Introduction
Uranium-based fuels have been used for space reactor applications for many years. In particular, uranium dioxide (UO2) has played an important role as fuel for the TOPAZ space reactors. Therefore, a sound understanding of the U–O system is required for the design, operation and disposal of reactor fuels for space applications.
Oxidation of UO2 (due to a reaction with air or steam, for example) may result in the formation of higher oxides, such as U4O9, U3O7 and U3O8[1] depending on the temperature and oxygen partial pressure. The change in density, crystal structure and chemical behaviour accompanying the introduction of these higher phases may have adverse effects on the mechanical and chemical performance of the fuel. Therefore, it is important to understand the stability of the various phases present.
Many investigators have studied the U–O system, most recently summarized by Guéneau et al. [2], Chevalier et al. [3] and Lewis et al. [4] as UO2 has traditionally been a popular fuel for both military and commercial water-cooled power reactors. Therefore, the U–O phase diagram is fairly well established. There still exists, however, some uncertainty around the non-stoichiometry of U4O9. Recent attempts to model the U–O system [3] approximate U4O9 as stoichiometric. Many investigators, however, have shown that U4O9 is a narrowly non-stoichiometric phase (U4O9−y). Experiments have shown that three phases exist: α-U4O9−y (below ∼80 °C), β-U4O9−y (between ∼80 °C and ∼550 °C) and γ-U4O9−y (above ∼550 °C) [5]. Fig. 1 shows a summary of the experimental data [6], [7], [8], [9], [10], [11], [12], [13], [14], [15], [16], [17], [18], [19] on the location of the phase boundaries for U4O9−y as well as the proposed fields for the three phases of U4O9−y overlaid on the current thermodynamic treatment for this system [20]. In addition, the kinetics of precipitation of U4O9 from UO2+x are not well known, only that quenching of UO2+x is required to prevent the formation of U4O9[6], [19].
Section snippets
Description of experiment
To investigate the non-stoichiometry in U4O9 and the kinetics of precipitation of U4O9 from UO2+x, an in situ neutron diffraction experiment was performed using the high-pressure preferred orientation (HIPPO) neutron diffractometer [21], [22] at the Los Alamos Neutron Science Center (Los Alamos National Laboratory, New Mexico).
The reason neutron diffraction is used instead of X-ray diffraction (XRD) for the study of the U–O system is due to the much deeper penetrating depth into UO2 with
Data analysis
Rietveld refinement [23] of the diffraction patterns was performed using the General Structure Analysis System (GSAS) software [24]. Diffuse scattering parameters were included to account for the silica glass liner (container). The crystal structures used in the refinement were stoichiometric UO2 space group Fm3m from Hutchings [25] and UO2.234 space group I3d from Kim et al. [26]. The observed patterns also matched the I3d structure reported by Copper and Wills [27]. Many other crystal
Discussion of results
One result from this experiment of particular interest is the weight fraction of UO2 at the beginning of the experiment (Fig. 5) and its accompanying lattice parameter (Fig. 6). On the initial heat up of the sample, the UO2 phase weight fraction is much higher (∼100% instead of ∼30%) and its lattice constant is lower than would be expected from the phase diagram and published lattice parameter data for stoichiometric UO2 (this can also visually seen from the patterns in Fig. 3). These results
Conclusions
The excellent agreement of refined lattice parameters and weight fractions from the neutron diffraction experiment with published values has demonstrated that time-of-flight neutron diffraction can be a very useful tool for studies of the U–O system, even at high temperatures. The neutron diffraction experiment has demonstrated that, at approximately 300 °C, a powder sample of UO2+x will reach thermodynamic equilibrium in less than 1 h and U4O9−y can begin to precipitate at only 100 °C. In
Acknowledgements
The authors would like to acknowledge the helpful discussions with S. White (RMC) and experimental support of D. Williams and O. Gourdon (LANL). The sample for this study was provided by J. Dunwoody (LANL). The work was funded in part by the National Science and Engineering Research Council of Canada (NSERC).
This work has benefited from the use of the Los Alamos Neutron Science Center at the Los Alamos National Laboratory. This facility is funded by the US Department of Energy under Contract
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