We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

We review the present status of the experimental and theoretical developments in the field of
strangeness in nuclei and neutron stars. We start by discussing the K ̄ N interaction, that is …

Recent progress in the determination of both masses and radii of neutron stars has put
strong constraints on the equation of state (EoS) above the nuclear saturation density. Within …

This study simulates strange stars in f (Q) gravity with an additional source under an electric
field using gravitational decoupling by means of the complete geometric deformation (CGD) …

I review holographic models for (dense and cold) nuclear matter, neutron stars, and their
mergers. I start by a brief general discussion on current knowledge of cold QCD matter and …

In this work we study the properties of compact spheres made of a charged perfect fluid with
a MIT bag model EoS for quark matter. Considering static spherically symmetric spacetime …

The current trend concerning dense matter physics at sufficiently high densities and low
temperatures is expected to behave as a degenerate Fermi gas of quarks forming Cooper …

Recent advances in nuclear theory and new astrophysical observations have led to the
need for specific theoretical models applicable to dense-matter physics phenomena …

Glitches, spin-up events in neutron stars, are of prime interest, as they reveal properties of
nuclear matter at subnuclear densities. We numerically investigate the glitch mechanism …

In order to extract the precise physical information encoded in the gravitational and
electromagnetic signals from powerful neutron-star merger events, we need to include as …