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We explore neutron skin predictions for $^{208}$Pb in relation to thesymmetry pressure in various microscopic models based on realisticnucleon-nucleon potentials and either the Dirac-Brueckner-Hartree-Fock approachor the conventional Brueckner-Hartree-Fock framework implemented withthree-body forces. We also discuss the correlation between the neutron skin andthe radius of a fixed-mass neutron star.

The neutron skin of $^{208}$Pb and the density dependence of the symmetry energy