“…This is particularly true for point defects, which have been demonstrated to be predominantly formed during collision cascades [4,5,25]. For instance, migration barrier values of 0.32 eV and 0.40 eV for O and Mg single-interstitials [4,5,25] and between 0.06, 0.33 and 1.04 eV for O À , O 2À and O 0 single-interstitials [28] were computed. In [4,5,25], di-interstitials and tri-interstitials were also found to be mobile at RT, but the migration barrier increases with the cluster size making them immobile at RT, except for the peculiar hexa-interstitial cluster with a diffusion barrier of 0.24 eV.…”