Abstract

The relativistic Hartree approach describing the bound states of both nucleons and antinucleons in finite nuclei has been extended to include tensor couplings for the $\ensuremath{\omega}$ and $\ensuremath{\rho}$ mesons. After readjusting the parameters of the model to the properties of spherical nuclei, the effect of tensor-coupling terms raises the spin-orbit force by a factor of 2, while a large effective nucleon mass ${m}^{*}{/M}_{N}\ensuremath{\approx}0.8$ sustains. The overall nucleon spectra of shell-model states are improved evidently. The predicted antinucleon spectra in the vacuum are deepened about 20--30 MeV.

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