Relativistic Hartree equations for spherical nuclei have been derived from a
relativistic quark model of the structure of bound nucleons which interact
through the (self-consistent) exchange of scalar (σ) and vector
(ω and ρ) mesons. The coupling constants and the mass of the
σ-meson are determined from the properties of symmetric nuclear matter
and the rms charge radius in 40Ca. Calculated properties of static,
closed-shell nuclei from 16O to 208Pb are compared with experimental
data and with results of Quantum Hadrodynamics (QHD). The dependence of the
results on the nucleon size and the quark mass is investigated. Several
possible extensions of the model are also discussed.Comment: 37 pages, 17 postscript figures are included, uses epsfig.sty,
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