# Reduced-Order Modelling of Defect Transport using Surrogate Kinetics: Application to U$\_x$Pu$\_ {1-x}$N

Source: [Reduced-Order Modelling of Defect Transport using Surrogate Kinetics: Application to U$\_x$Pu$\_ {1-x}$N](<https://www.sota2.com/research/paper/6a3a13b6206542251d7c7895>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2026-06-24T05:00:31.418Z

Authors: Peter Hatton

Published: 2026-06-22T10:15:22.000Z

## Abstract

Defect transport in chemically disordered materials is a difficult phenomenon to model since migration energetics depend strongly on the local chemical environment, producing a distribution of transition barriers that cannot be exhaustively enumerated. Here, we develop a reduced-order approach to modelling defect diffusion in compositionally complex materials using environment-dependent surrogate kinetics. Migration energetics for actinide vacancies, nitride vacancies, and actinide-nitride divacancies in U$\_x$Pu$\_{1-x}$N are generated using the Hop-Decorate workflow across thousands of chemical configurations. These data are distilled into compact surrogate functions that predict migration barriers and energy differences from simple descriptors based on local coordination counts. The surrogate models reproduce the atomistic dataset with low error and enable efficient evaluation of migration rates during lattice kinetic Monte Carlo simulations. Long-time diffusivities computed across temperature and composition reveal strongly non-linear behaviour arising from two dominant mechanisms: species-controlled migration on the actinide sublattice and environment-dependent trapping on the nitride sublattice. Although demonstrated for U$\_x$Pu$\_{1-x}$N the framework provides a general and computationally efficient approach for modelling defect transport in chemically disordered materials and for integrating atomistic kinetics into higher-scale simulations.

## Recorded benchmark results

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## Original sources and implementation

[Original paper](<https://arxiv.org/abs/2606.23128>)

[PDF](<https://arxiv.org/pdf/2606.23128.pdf>)