Characterization of radiation defects in austenitic alloys

Condensed matter physics

Numerical calculation of formation energy of different radiation defects at zero temperature (T = 0 K) in the austenitic Fe0.7Ni0.1Cr0.2 model alloy using classical molecular dynamics method has been carried out. Thermal stability of the radiation defects by means of annealing modeling at different non-zero temperatures was studied.