The reflectivity and reflectance anisotropy (RA) spectra of five silic
on surfaces [(001), (113), (112), (111), and (110)] are calculated usi
ng the discrete dipole model. The structures used have bulk-terminated
surfaces so that RA is found at the optical gap and above. A comparis
on is made between experimental RA spectra of H-covered (001), (113),
and (110) surfaces and-the discrete dipole spectra, and it is found th
at there is agreement for the (001) and (110) surfaces but the best fi
t to the experimental (113) surface spectrum is found for a (112) surf
ace discrete dipole calculation. RA spectra are obtained using the McI
ntyre-Aspnes three-layer model with surface layer and bulk dielectric
functions taken from discrete dipole calculations. Surface excess diel
ectric functions are shown for these surfaces. It is found that, altho
ugh RA spectra of the different surfaces are quite distinct, the gross
features of the surface excess dielectric functions that are used to
calculate them are quite similar. Thus small shifts in maxima and mini
ma and differences in strength of these functions are responsible for
the observed optical anisotropy, rather than distinct spectral feature
s that differ from surface to surface. The surface dielectric function
converges to the bulk value within 10 to 20 Angstrom of the vacuum-so
lid interface, depending on frequency, so that RA at frequencies corre
sponding to the optical gap energy and above arises from this 20 Angst
rom region, rather than the topmost surface layer or layers.