A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

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 …

We investigate the implications of parity-violating electron scattering experiment on neutron
skin thickness of Ca 48 [calcium radius experiment (CREX)] and Pb 208 [lead radius …

This guide offers suggestions/insights on uncertainty quantification of nuclear structure
models. We discuss a simple approach to statistical-error estimates, strategies to assess …

Background: Theoretical approaches based on density functional theory provide the only
tractable method to incorporate the wide range of densities and isospin asymmetries …

Background: Nuclear density functional theory is the only microscopical theory that can be
applied throughout the entire nuclear landscape. Its key ingredient is the energy density …

The complex nature of the nuclear forces generates a broad range and diversity of
observational phenomena. Heavy nuclei, though orders of magnitude less massive than …

Differences in the charge radii of mirror nuclei have been recently suggested to contain
information on the slope of the symmetry energy L. To test this hypothesis, we perform …

The critical densities and impact of forming Δ (1232) resonances in neutron stars are
investigated within an extended nonlinear relativistic mean-field (RMF) model. The critical …

Background: The first direct detection of a binary neutron star merger by the LIGO Scientific
Collaboration and the Virgo Collaboration (LIGO-Virgo)[Phys. Rev. Lett. 119, 161101 (2017) …