Abstract

Nuclear equation of state is often described in the framework of energy density functional. However, the isovector channel in most functionals has been poorly constrained, mainly due to rather limited available experimental data to probe it. Only recently, the relativistic nuclear energy density functional with an effective point-coupling interaction was constrained by supplementing the ground-state properties of nuclei with the experimental data on dipole polarizability and isoscalar monopole resonance energy in 208Pb, resulting in DD-PCX parameterization. In this work, we pursue a complementary approach by introducing a family of 8 relativistic point-coupling functionals that reproduce the same nuclear ground-state properties, including binding energies and charge radii, but in addition have a constrained value of symmetry energy at saturation density in the range J = 29, 30, …, 36 MeV. In the next step, this family of functionals is employed in studies of excitation properties such as dipole polarizability and magnetic dipole transitions, and the respective experimental data are used to validate the optimal choice of functional as well as to assess reliable values of the symmetry energy and slope of the symmetry energy at saturation.

Highlights

  • We present the results for the nuclear matter properties in relation to the electric and magnetic dipole excitation properties using the new family of pointcoupling functionals spanning the range of values for the symmetry energy at saturation

  • We present our calculations using the DD-PC family of functionals varying the J value as well as the DD-PC1 and DD-PCX ones, and the theoretical results using the other functionals were taken from Reference [60]

  • Constraining the isovector channel of the energy density functional (EDF), which is of paramount importance for description of the symmetry energy of the nuclear equation of state (EoS), represents a continuous challenge for the nuclear physics and astrophysics community

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Summary

Introduction

The EoS around saturation density is often constrained by the ground-state properties of finite nuclei, and the nuclear excitation properties provide valuable information to optimize the EDFs used in the description of the EoS. The properties of symmetric nuclear matter around saturation are rather well-constrained by fitting the model parameters to the ground-state observables of nuclei. These observables are not able to constrain well the isovector channel of the functionals, which in turn leads to poorly constrained symmetry energy parameters of the EoS, and additional constraints on the pseudo-observables on the nuclear matter are introduced to cure this deficiency.

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