Symmetry energy effects on isovector properties of neutron rich nuclei with a Thomas-Fermi approach

Abstract

We employ a variational method, in the framework of the Thomas-Fermi approximation, to study the effect of the symmetry energy on the neutron skin thickness and the symmetry energy coefficients of various neutron rich nuclei. We concentrate our interest on ${}^{208}$Pb, ${}^{124}$Sn, ${}^{90}$Zr, and ${}^{48}$Ca, although the method can be applied in the totality of medium and heavy neutron rich nuclei. Our approach has the advantage that the isospin asymmetry function $\alpha (r)$, which is the key quantity to calculate isovector properties of various nuclei, is directly related with the symmetry energy as a consequence of the variational principle. Moreover, the Coulomb interaction is included in a self-consistent way and its effects can be separated easily from the nucleon-nucleon interaction. We confirm, both qualitatively and quantitatively, the strong dependence of the symmetry energy on the various isovector properties for the relevant nuclei, using possible constraints between the slope and the value of the symmetry energy at the saturation density.

19 pages, 12 figures, 1 table

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Cited by in corpus (2)

• EoS constraints from nuclear masses and radii in a meta-modeling approach
• Nuclear skin and the curvature of the symmetry energy