Collision cascades in metals produce small interstitial clusters and perfec
t dislocation loops that glide in thermally activated one-dimensional (1D)
random walks. These gliding defects can change their Burgers vectors by the
rmal activation or by interactions with other defects. Their migration is t
herefore 'mixed 1D/3D migration' along a 3D path consisting of 1D segments,
The defect reaction kinetics under mixed 1D/3D diffusion are different fro
m pure 1D diffusion and pure 3D diffusion, both of which can be formulated
within analytical rate theory models of microstructure evolution under irra
diation. Atomic-scale kinetic Monte Carlo (kMC) defect migration simulation
s are used to investigate the effects of mixed 1D/3D migration on defect re
action kinetics as a guide for implementing mixed 1D/3D migration into the
analytical rate theory. The functional dependence of the sink strength on t
he size and concentration of sinks under mixed 1D/3D migration is shown to
lie between that for pure 1D and pure 3D migration and varies with L, the a
verage distance between direction changes of the gliding defects. It is sho
wn that the sink strength in simulations for spherical sinks of radius R un
der mixed 1D/3D migration for values of L greater than R can be approximate
d by an expression that varies directly as R-2. For small L, the form of th
e transition from mixed 1D/3D to pure 3D diffusion as L decreases is demons
trated in the simulations, the results of which can be used in the future d
evelopment of an analytical expression describing this transition region. (
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