In recent years our understanding of neutron stars has advanced remarkably, thanks to
research converging from many directions. The importance of understanding neutron star …

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 …

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 …

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 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 …

A wide variety of experimental results and theoretical investigations in recent years have
convincingly demonstrated that several transition metal oxides and other materials have …

A statistical model for the equation of state and the composition of supernova matter is
presented. It consists of an ensemble of nuclei and interacting nucleons in nuclear statistical …

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 …

Many fundamental issues in classical condensed matter physics can be addressed
experimentally using systems of individually visible mesoscopic particles playing the role of …