Abstract
In separate publications we have, from a variety of considerations, identified the activation enthalpies for migration by nearest-neighbor hopping, ΔHm, of vacancies in InP as ΔHm(VIn)=0.3 eV and ΔHm(VP)=1.2 eV. These are in the ratio of the masses of the P and In atoms that actually move when VIn’s and VP’s hop to nearest-neighbor sites. Here we argue that this is evidence for the validity of the kinetic interpretation of ΔHm and the ballistic model of vacancy migration. Indeed, the empirical values are in quantitative agreement with the predictions of the ballistic model. Excellent agreement is also found for VMg migration in MgO. We extrapolate this result to predict that high-temperature values for interstitial migration in Si and other tetrahedral semiconductors will also be dominated by a kinetic-energy term and far larger than low-temperature values are known to be.