Francesca Sammarruca, Pei Liu
Published 2008-12-29, updated 2009-01-19Version 2
We explore neutron skin predictions for $^{208}$Pb in relation to the symmetry pressure in various microscopic models based on realistic nucleon-nucleon potentials and either the Dirac-Brueckner-Hartree-Fock approach or the conventional Brueckner-Hartree-Fock framework implemented with three-body forces. We also discuss the correlation between the neutron skin and the radius of a fixed-mass neutron star.
Comments: 12 pages, 12 figures. Submitted to Physical Review C
Journal: Phys.Rev.C79:057301,2009
Probing the density dependence of symmetry energy at subsaturation density with HICs
Constraining the density dependence of the symmetry energy using the multiplicity and average $p_T$ ratios of charged pions
Density dependence of the "symmetry energy" in the lattice gas model
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