Ab initio molecular dynamics simulations are employed to investigate t
he dominant migration mechanism of the gallium vacancy in GaAs as well
as to assess its free energy of formation and the rate constant of ga
llium self-diffusion. Our analysis suggests that the vacancy migrates
by second-nearest neighbour hops. The calculated self-diffusion consta
nt is in good agreement with the experimental value obtained in (GaAs)
-Ga-69/(GaAs)-Ga-71 isotope heterostructures and at significant varian
ce with that obtained earlier from interdiffusion experiments in GaAlA
s/GaAs-heterostructures.