The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

Transport models are the main method to obtain physics information on the nuclear equation
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …

Investigation into the properties and structure of unstable nuclei far from stability is a key
avenue of research in modern nuclear physics. These efforts are motivated by the continual …

We confront observational data from gravitational wave event GW170817 with microscopic
modeling of the cold neutron star equation of state. We develop and employ a Bayesian …

Various kinds of isovector nucleon effective masses are used in the literature to characterize
the momentum/energy dependence of the nucleon symmetry potential or self-energy due to …

Recent precise parity-violating electron scattering experiments on 48 Ca (CREX) and 208
Pb (PREX-II) provide a new insight on the formation of neutron skin in nuclei. Within the …

Background: Very lately, the CREX group presents a skin value Δ R skin 48 (CREX)= 0.
121±0. 026 (exp)±0. 024 (model)= 0. 071∼ 0. 171 fm. Meanwhile, the PREX group reported …

We present predictions for neutron star tidal deformabilities obtained from a Bayesian
analysis of the nuclear equation of state, assuming a minimal model at high-density that …

We introduce a new relativistic energy density functional constrained by the ground state
properties of atomic nuclei along with the isoscalar giant monopole resonance energy and …

We derive the empirical formulas expressing the mass and gravitational redshift of a neutron
star, whose central density is less than threefold the nuclear saturation density, as a function …