The general behavior of the nuclear equation of state (EOS), relevant for the description of
neutron stars (NSs), is studied within a Bayesian approach applied to a set of models based …

Gravitational-wave (GW) detections of binary black hole (BH) mergers have begun to
sample the cosmic BH mass distribution. The evolution of single stellar cores predicts a gap …

The impacts of various symmetry energy parameters on the properties of neutron stars (NSs)
have been recently investigated, and the outcomes are at variance, as summarized in Table …

Binary neutron-star mergers and heavy-ion collisions are related through the properties of
the hot and dense nuclear matter formed during these extreme events. In particular, low …

A modified version of the density dependent covariant density-functional model proposed in
[Astrophys. J. 930, 17 (2022) 10.3847/1538-4357/ac5d3c] is employed in a Bayesian …

Over the last few years, researchers have become increasingly interested in understanding
how dark matter affects neutron stars, helping them to better understand complex …

We analyze the uncertainties introduced in the determination of the neutron star matter
proton fraction, in a range of densities close to the saturation density, if the cold β …

We analyze the implications of information about local derivatives from the mass-radius
diagram in neutron star matter. It is expected that the next generation of gravitational wave …

Resonant shattering flares (RSFs) are bursts of gamma-rays expected to be triggered by
tidal resonance of a neutron star (NS) during binary inspiral. They are strongly dependent on …

The effects on the speed of sound in neutron stars due to the presence of hyperons and a
phase transition to deconfined quark matter is investigated. For this purpose a composite …