  We derive the values of nuclear symmetry energy, its components, as well as
pressure in finite nuclei at saturation density from their corresponding values
in nuclear matter obtained in non-relativistic Brueckner-Hartree-Fock
calculations with the realistic Bonn B and Bonn CD potentials using the
coherent density fluctuation model in the framework of a self-consistent
Skyrme-Hartree-Fock plus BCS method. We focus on three isotopic chains of
spherical nuclei (Ni, Sn, and Pb) and compare our results with those obtained
with an effective Brueckner density-dependent potential. The role of the
three-body forces on the considered quantities is also studied and discussed.
