According to the production bias model, glissile defect clusters and small
dislocation loops play an important role in the microstructural evolution d
uring irradiation under cascade damage conditions. The atomic scale compute
r simulations carried out in recent years have clarified many questions abo
ut the structure and properties of glissile clusters of self-interstitial a
toms that are formed directly in the cascade volume. It has been found that
such clusters consist of sets of crowdions and are highly mobile in the cr
owdion direction. Very recently, one-dimensional glide of similar character
has been observed in the computer simulation of small vacancy loops in alp
ha-Fe. In the present paper we summarise results obtained by molecular dyna
mics simulations of defect clusters and small dislocation loops in alpha-Fe
(bcc) and Cu(fcc). The structure and stability of vacancy and interstitial
loops are reviewed, and the dynamics of glissile clusters assessed. The rel
evance and importance of these results in establishing a better understandi
ng of the observed differences in the damage accumulation behaviour between
bcc and fee metals irradiated under cascade damage conditions are pointed
out. (C) 2000 Elsevier Science B.V. All rights reserved.