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 …

Advances in our understanding and the modeling of stellar core-collapse and supernova
explosions over the past 15 years are reviewed, concentrating on the evolution of …

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 …

We investigate the causal limit of maximum mass for stars in the framework of f (R) gravity.
We choose a causal equation of state, with variable speed of sound, and with the transition …

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 …

In this work, we study the neutron star phenomenology of R p attractor theories in the
Einstein frame. The Einstein frame R p attractor theories have the attractor property that they …

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 …

Observations of magnetars and some of the high magnetic field pulsars have shown that
their thermal luminosity is systematically higher than that of classical radio-pulsars, thus …

The physics of neutron star crusts is vast, involving many different research fields, from
nuclear and condensed matter physics to general relativity. This review summarizes the …

In this work we study static neutron stars in the context of several inflationary models which
are popular in cosmology. These inflationary models are nonminimally coupled scalar …