Correlated structure of nuclear symmetry energy from covariant nucleon self-energy
arXiv:1809.03837
Abstract
Based on the Hugenholtz-Van Hove theorem, the symmetry energy and its density slope parameter are decomposed in terms of the nucleon self-energies within the covariant density functional (CDF) theory. It is found that two structural connections between the different ingredients of and construct the fundamental correlation between and in the relativistic covariant framework, while the additional contribution from the isovector scalar channel of nucleon-nucleon interaction and those from the second-order symmetry self-energies lead to a deviation, especially the latter limits severely its correlation coefficient and confidence level. In addition, the relationship between the Landau mass and the Dirac mass is approximated to a reliable linear correlation, which is demonstrate to be sensitive to the momentum dependence of the nucleon self-energies.
arXiv comment10 pages, 5 figures, corresponding to the talk given in NuSYM2018
References in corpus (30)
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Equations of state for supernovae and compact stars
- Reaction Dynamics with Exotic Beams
- New parametrization for the nuclear covariant energy density functional with point-coupling interaction
- Skyrme Interaction and Nuclear Matter Constraints
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- The maximum mass and radius of neutron stars and the nuclear symmetry energy
- Constraints on the symmetry energy and on neutron skins from the pygmy resonances in 68Ni and 132Sn
- A way forward in the study of the symmetry energy: experiment, theory, and observation
- Density-Dependent Relativistic Hartree-Fock Approach
- Core-crust transition in neutron stars: predictivity of density developments
- Relativistic mean field interaction with density dependent meson-nucleon vertices based on microscopical calculations
- Relativistic model for nuclear matter and atomic nuclei with momentum-dependent self-energies
- Beta-decay rates of r-process nuclei in the relativistic quasiparticle random phase approximation
- Neutron star properties in density-dependent relativistic Hartree-Fock theory
- Divergence of the isospin-asymmetry expansion of the nuclear equation of state in many-body perturbation theory
- Calculation of beta-decay rates in a relativistic model with momentum-dependent self-energies
- Interdependence of different symmetry energy elements
- Single-nucleon potential decomposition of the nuclear symmetry energy
- Analytical relations between nuclear symmetry energy and single-nucleon potentials in isospin asymmetric nuclear matter
- The Nuclear Tensor Interaction in Covariant Energy Density Functional
- Properties of dense, asymmetric nuclear matter in Dirac-Brueckner-Hartree-Fock approach
- Universal correlations in the nuclear symmetry energy, slope parameter, and curvature
- Extracting the nuclear symmetry potential and energy from neutron-nucleus scattering data
- Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
- Lorentz covariant nucleon self-energy decomposition of the nuclear symmetry energy
- Correlations between the nuclear matter symmetry energy, its slope, and curvature from a nonrelativistic solvable approach and beyond
- Relativistic interpretation on the nature of nuclear tensor force
- Symmetry Energy
- Universal symmetry energy contribution to the neutron star equation of state