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 …

This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …

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 …

Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …

We present a critical assessment of the SN1987A supernova cooling bound on axions and
other light particles. Core collapse simulations used in the literature to substantiate the …

The detection of GW170817 in gravitational waves provides unprecedented constraints on
the equation of state (EOS) of the ultradense matter within the cores of neutron stars (NSs) …

The uncertainties in neutron star radii and crust properties due to our limited knowledge of
the equation of state are quantitatively analyzed. We first demonstrate the importance of a …

This paper presents a detailed assessment of the ability of the 240 Skyrme interaction
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …

The information on the symmetry energy and its density dependence is deduced by
comparing the available data on the electric dipole polarizability α D of Ni 68, Sn 120, and …

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