The density dependence of nuclear symmetry energy is among the most uncertain parts of
the Equation of State (EOS) of dense neutron-rich nuclear matter. It is currently poorly known …

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …

Constraints set on key parameters of the nuclear matter equation of state (EoS) by the
values of the tidal deformability, inferred from GW170817, are examined by using a diverse …

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 …

We investigate the impact of the neutron-star matter equation of state on the f-and p 1-mode
oscillations of neutron stars obtained within the Cowling approximation and linearized …

Within the parameter space of the equation of state (EOS) of dense neutron-rich matter
limited by existing constraints mainly from terrestrial nuclear experiments, we investigate …

The tidal measurement of gravitational waves from the binary neutron star merger event
GW170817 allows us to probe nuclear physics that suffers less from astrophysical …

We use covariant density functional theory to obtain the equation of state (EoS) of matter in
compact stars at non-zero temperature, including the full baryon octet as well as the Δ …

In this work, we propose a metamodeling technique to nuclear matter on the basis of a
relativistic density functional with density-dependent couplings. Identical density …

The impacts of various symmetry energy parameters on the properties of neutron stars (NSs)
have been recently investigated, and the outcomes are at variance, as summarized in Table …