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 …

The nuclear symmetry energy characterizes the variation of the binding energy as the
neutron to proton ratio of a nuclear system is varied. This is one of the most important …

Is the secondary component of GW190814 the lightest black hole or the heaviest neutron
star ever discovered in a double compact-object system [Abbott et al. Astrophys. J. 896, L44 …

An accurately calibrated relativistic parametrization is introduced to compute the ground
state properties of finite nuclei, their linear response, and the structure of neutron stars …

Neutrinos are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …

Core-collapse supernovae are among the most energetic explosions in the universe
marking the catastrophic end of massive stars. In spite of rigorous studies for several …

We discuss the consequences of the accretion of dark matter (DM) particles on compact
stars such as white dwarfs and neutron stars. We show that in large regions of the DM …

The transition density ρ t and pressure P t at the inner edge separating the liquid core from
the solid crust of neutron stars are systematically studied using a modified Gogny (MDI) and …

Nuclear pasta, with nonspherical shapes, is expected near the base of the crust in neutron
stars. Large-scale molecular dynamics simulations of pasta show long lived topological …

We present the potential sensitivity of a future recoil detector for a first detection of the
process of coherent elastic neutrino nucleus scattering (CEνNS). We use the Chooz reactor …