We use molecular dynamics computer simulations to study the equilibrium pro
perties of the surface of amorphous silica. Two types of geometries are inv
estigated: (i) clusters with different diameters (13.5, 19, and 26.5 Angstr
om) and (ii) a thin film with thickness 29 Angstrom. We find that the shape
of the clusters is independent of temperature and that it becomes more sph
erical with increasing size. The surface energy is in qualitative agreement
with the experimental value for the surface tension. The density distribut
ion function shows a small peak just below the surface, the origin of which
is traced back to a local chemical ordering at the surface. Close to the s
urface the partial radial distribution functions as well as the distributio
ns of the bond-bond angles show features which are not observed in the inte
rior of the systems. By calculating the distribution of the length of the S
i-O rings we can show that these additional features are related to the pre
sence of two-membered rings at the surface. The surface density of these st
ructures is around 0.6/nm(2), in good agreement with experimental estimates
. From the behavior of the mean-squared displacement at low temperatures, w
e conclude that at the surface the cage of the particles is larger than the
one in the bulk. Close to the surface the diffusion constant is somewhat l
arger than the one in the bulk and with decreasing temperature the relative
difference grows. The total vibrational density of states at the surface i
s similar to the one in the bulk. However, if only the one for the silicon
atoms is considered, significant differences are found. (C) 2001 American I
nstitute of Physics.