The atomistic simulations in the framework of the Generalized Simulated Ann
ealing approach (GSA) and classical force fields lead to very reasonable re
laxed geometries around the carbon interstitial in O-, T-, and TS-sites. We
have thus shown that a highly efficient energy-sampling and relaxation sch
eme, implemented with tight constraints on a limited volume, provides a pow
erful steering mechanism for selection of geometries suitable for detailed
investigation by first-principles methods. The results, based upon harmonic
interactions between Cu atoms and a van der Waals interaction between Cu a
nd C, predict the relaxed O-site to be more stable than the T-site by simil
ar to 1.2 eV, in accordance with general expectations. The TS barrier to O-
O diffusion is found to be similar to 0.8 eV, at a temperature of 0 K; the
TS exhibits a strong local axial distortion of the pseudo-octahedral enviro
nment. The Density Functional results indicate a charge transfer of similar
to 1 e to carbon, mostly from the first neighbor shell, in all relaxed env
ironments studied. Bond-order data show the Cu-C interaction to be bonding
in nature, despite the net 'repulsive interaction' leading to a surface sta
te of lower net energy. (C) 2000 Elsevier Science Ltd. All rights reserved.