Bao-Jun Cai

Higher-order effects on the incompressibility of isospin asymmetric nuclear matter

Analytical expressions for the saturation density of asymmetric nuclear matter as well as its binding energy and incompressibility at saturation density are given up to fourth order in the isospin asymmetry

Single-nucleon potential decomposition of the nuclear symmetry energy

\ensuremath{\delta}=({\ensuremath{\rho}}_{n}\ensuremath{-}{\ensuremath{\rho}}_{p})/\ensuremath{\rho}

Critical density and impact of Δ(1232) resonance formation in neutron stars

using 11 characteristic parameters defined by the density derivatives of the binding energy per nucleon of symmetric nuclear matter, the symmetry energy

Extracting the nuclear symmetry potential and energy from neutron-nucleus scattering data

{E}_{\mathrm{sym}} (\ensuremath{\rho})

Isospin quartic term in the kinetic energy of neutron-rich nucleonic matter

, and the fourth-order symmetry energy

Nucleon effective masses in neutron-rich matter

{E}_{\mathrm{sym},4}(\ensuremath{\rho})

Nucleon effective E-mass in neutron-rich matter from the Migdal–Luttinger jump

at normal nuclear density

Isospin dependence of nucleon effective masses in neutron-rich matter

{\ensuremath{\rho}}_{0}

Proton-skins in momentum space and neutron-skins in coordinate space in heavy nuclei

. Using an isospin- and momentum-dependent modified Gogny interaction (MDI) and the Skyrme-Hartree-Fock (SHF) approach with 63 popular Skyrme interactions, we have systematically studied the isospin dependence of the saturation properties of asymmetric nuclear matter, particularly the incompressibility

INCOMPRESSIBILITY OF ASYMMETRIC NUCLEAR MATTER

{K}_{\mathrm{sat}}(\ensuremath{\delta})={K}_{0}+{K}_{\mathrm{sat},2}{\ensuremath{\delta}}^{2}+{K}_{\mathrm{sat},4}{\ensuremath{\delta}}^{4}+O({\ensuremath{\delta}}^{6})