Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars

Zhen Zhang, Lie-Wen Chen

Published 2015-10-21Version 1

Recent progress in theory, experiment and observation challenges the mean field models using the conventional Skyrme interaction, suggesting that the extension of the conventional Skyrme interaction is necessary. In this work, we construct three Skyrme interaction parameter sets, namely, eMSL07, eMSL08 and eMSL09, based on an extended Skyrme interaction which includes additional momentum and density dependent two-body forces to effectively simulate the momentum dependence of the three-body force. The three new interactions can well reproduce both the ground-state properties and isoscalar giant monopole resonance energy of finite nuclei, nicely conform to the current knowledge on the equation of state of asymmetric nuclear matter around and below saturation density $\rho_0$, eliminate the notorious unphysical instabilities of symmetric nuclear matter and pure neutron matter at densities up to about $7.5\rho_0$, and simultaneously support heavier neutron stars with mass larger than two times solar mass. The new family of the extended Skyrme interactions can thus provide a unified description for the properties of asymmetric nuclear matter from sub- to supra-saturation densities in large region of isospin values and are appropriate for the study of nuclear matter, finite nuclei and neutron stars.