The nanostructure evolution in Fe-C systems under irradiation at 560 K
Ville Jansson, Monica Chiapetto, Lorenzo Malerba

TL;DR
This study extends a kinetic Monte Carlo model to simulate nanostructure evolution in Fe-C alloys at reactor-operational temperatures, capturing defect dynamics and the influence of carbon at higher irradiation temperatures.
Contribution
The paper introduces an adapted model that accounts for two types of SIA clusters and validates it against experimental data at 560 K, enhancing understanding of irradiation effects in Fe-C alloys.
Findings
Model reproduces experimental nanostructure trends
Carbon forms immobile vacancy complexes acting as SIA traps
Different SIA cluster types are observed and modeled
Abstract
This work extends our Object Kinetic Monte Carlo model for neutron irradiation-induced nanostructure evolution in Fe-C alloys to consider higher irradiation temperatures. The previous study concentrated on irradiation temperatures < 370 K. Here we study the evolution of vacancy and self-interstitial atom (SIA) cluster populations at the operational temperature of light water reactors, by simulating specific reference irradiation experiments. Following our previous study, the effect of carbon on radiation defect evolution can be described in terms of formation of immobile complexes with vacancies, that in turn act as traps for SIA clusters. This dynamics is simulated using generic traps for SIA and vacancy clusters. The traps have a binding energy that depends on the size and type of the clusters and is also chosen on the basis of previously performed atomistic studies. The model had…
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