Uranium nitride (UN) is a promising nuclear fuel for space reactors and accident-tolerant fuel (ATF) applications due to its high uranium density, high thermal conductivity, and high melting point. However, its rapid oxidation in oxygen-containing environments severely limits its practical use. Experimental observations have shown that UN oxidation proceeds through a U2N3 transition phase before eventually forming UO2, but the underlying atomic-scale mechanisms have not been fully elucidated.
In this work, we systematically investigate the initial oxidation behavior of UN, the metastable structural characteristics of U2N3, and the energetic and kinetic evolution during oxidation by combining first-principles density functional theory (DFT) and molecular dynamics (MD) simulations. UN surface models are constructed to study oxygen adsorption and vacancy migration using the nudged elastic band (NEB) method. For U2N3±x, we examine three representative compositions, including stoichiometric U2N3, hypo-stoichiometric U2N2.6, and hyper-stoichiometric U2N3.4. The randomness of point defects is quantified by the coefficient of variation, and the formation energies are calculated to assess thermodynamic stability. Diffusion coefficients of N and O are computed using mean square displacement (MSD) for U2N3Ox system at 600 ℃.
Our results show that the UN surface acts as a trap for nitrogen vacancies. Additionally, the diffusion of oxygen atoms into the bulk through a vacancy-mediated mechanism is kinetically feasible. Within the investigated compositions (U2N3, U2N2.6 and U2N3.4), all exhibit high configurational flexibility and rich metastability. In U2N2.6, the additional structural vacancies prefer a random distribution over clustering. In U2N3.4, the interstitial N atoms show no preference for specific positions and are highly flexible. Thermodynamically, the stability of U2N3Ox increases monotonically with oxygen content, indicating that the oxidation process is spontaneous. Electronically, oxygen introduction increases the oxidation states of both U and N, with U being more sensitive. Kinetically, the diffusion coefficients of both N and O in U2N3Ox decrease gradually with increasing oxygen content, although the decrease is modest and remains within the same order of magnitude (approximately 10–8 cm2/s). Oxygen diffuses slightly faster than nitrogen. In contrast, UN exhibits complex three-dimensional migration pathways involving both \langle 100\rangle and dual-atom cooperative \langle 100\rangle migration mechanisms, while U2N3 shows a much simpler vacancy-diffusion mechanism strictly along the \langle 100\rangle direction due to its regular network of structural vacancies.
Collectively, our findings elucidate that the widespread presence of U2N3 during the initial stage of UN oxidation arises not from its thermodynamic stability, but from its exceptional configurational flexibility, abundant metastable states, and low migration barriers. This work provides a microscopic understanding of the transition role of U2N3 in UN oxidation and offers atomic-scale parameters for developing oxidation kinetic models of UN fuels.