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14 декабря, 2021
As mentioned above, the microscopic mechanisms of oxygen diffusion vary as a function of stoichiometry in the actinide dioxides. A schematic view of the (simplified) possible mechanisms has been reported in Table 18. Dorado eta/.232 combining both experimental and theoretical approaches identified the oxygen migration as an interstitialcy mechanism.
For x < 0in MO2 _ x (hypostoichiometric dioxides), the dominant defects in urania and plutonia are the oxygen vacancies. Hence, the migration energy could
Table 18 Simplified view of the migration energies of oxygen as a function of stoichiometry in MO2 ±x
Eact. and Ef set for activation and formation energies, respectively. FP, V, and I set for Frenkel pair, vacancy, and interstitial, respectively. |
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Figure 30 Comparison between the experimental self-diffusion coefficients of oxygen in hyperstoichiometric UO2 + x and the calculated ones at 1073 K. From Andersson, D. A.; Watanabe, T.; Deo, C.; Uberuaga, B. P. Phys. Rev. 2009, 806, 060101. |
be reduced to the activation energy for oxygen vacancy migration Eact: ( V") as reported in the Table 18.
In fact, Stan eta/.150’152 have shown that the point defects in hypostoichiometric plutonia PuO2 _ x do not reduce to oxygen vacancy. They determined (from a point defect model) that five different defects are at work in PuO2 _ x and hence contribute to the formation of oxygen vacancies. According to them, the prefactor D0 (eqn [13]) can then be written as a function of (i) a stoichiometry-dependent correlation factor from Tahir-Kheli233 and (ii) the formation energy of oxygen vacancy (determined using the point defect model). The results of such a model are reported in Figure 29.
Recently Kato et а/23 have studied the oxygen diffusion in hypostoichiometric MOX, and they
concluded that the diffusion coefficient of oxygen linearly depends upon the concentration of Pu in MOX.
For x > 0 in MO2 + x (hyperstoichiometric dioxides), two recent studies evidenced that the oxygen interstitials are not the only contribution to oxygen diffusion. Experimental data obtained by Ruello et a/.229 in UO2 + x show the important role of the Willis clusters. Theoretical calculations based on coupled ab initio/kinetic Monte Carlo done by Andersson et a/.168 have shown also that the diinterstitial cluster of oxygen may contribute to the oxygen diffusion for highly hyperstoichiometric UO2 + x. In fact, the diffusion of oxygen in hyperstoichiometric dioxides is due to the diffusion of interstitial oxygen and to the (counteracting) contribution of more complex oxygen clusters. Hence, the diffusion coefficient increases with stoichiometry, reaches a maximum, and decreases as may be seen in Figure 30.
Recently, Stan et a/.153 proposed a semiempirical relation between the diffusion coefficient D and the stoichiometry for UO2 + x that includes a maximum:
D(T, x) = xDo exp ^_Y°^j exp(_0x) [14]
In this expression, D0 = 1.3 x 10-2 cm2 s_1, E0 = 1.039 eV, and в = 6.1. The last term of the product corresponds to the blocking effect of the complex oxygen clusters. Such a semiempirical model reproduces the experimental data fairly well (see Figure 31), up to x < 0.1. For higher values of x (0.0 < x< 0.2 from 300 up to 1800 K), Ramirez eta/.151 established a somewhat different semiempirical relation.