A kinetic rate theory model, which includes the formation of cascade-induce
d clusters (CIIC), is presented. Comparison of the model to ion irradiation
data on vanadium reveals the effects of helium generation and cascade-indu
ced interstitial and vacancy clusters on microstructure evolution. The mode
l is based on a simplification of hierarchical rate equations for the clust
ering of helium bubbles, immobile vacancy clusters, glissile interstitial c
lusters, sessile dislocation loops, as well as precipitates and grain bound
aries. The model shows that the transport of helium to dislocations, bubble
s and grain boundaries is strongly transient because of coupling between th
e nucleation and growth modes of bubble evolution. Helium agglomeration in
vacancy clusters is shown to reduce the excess vacancy flux to grow matrix
and precipitate-affixed bubbles. The direct formation of vacancy and inters
titial clusters in cascades reduces the growth rate of bubbles, and leads t
o enhanced nucleation of matrix bubbles. In addition to the dislocation and
production bias mechanisms, a new mechanism of 'helium nucleation bias' is
shown to exist under high helium generation rates. (C) 2000 Elsevier Scien
ce B.V. All rights reserved.