The nucleon self-energy obtained from the Dirac Brueckner-Hartree-Fock
calculation is parametrized by introducing density-dependent coupling
constants of isoscalar mesons in the relativistic Hartree-Fock (RHF)
approach. The RHF calculations with density-dependent coupling constan
ts not only reproduce the nuclear matter saturation properties, but al
so provide a good starting point to study finite nuclei properties. Th
e relativistic density-dependent Hartree-Fock (RDHF) approach contains
the features of the relativistic G matrix and in the meantime simplif
ies the calculation. The ground state properties of spherical nuclei c
alculated in the RDHF are in good agreement with the experimental data
. The contribution of isovector mesons pi and rho, especially the cont
ribution of the tenser coupling of rho mesons, are discussed in this p
aper.