The density dependence of nuclear symmetry energy is among the most uncertain parts of
the Equation of State (EOS) of dense neutron-rich nuclear matter. It is currently poorly known …

We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

We use Stergioulas's RNS code for investigating fast pulsars with equations of state (EOSs)
on the causality surface (where the speed of sound is equal to that of light) of the high …

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 …

The radius R 1.4 of neutron stars (NSs) with a mass of 1.4 M⊙ has been extracted
consistently in many recent studies in the literature. Using representative R 1.4 data, we infer …

We examine the possibility that the light companion in the highly asymmetric binary compact
object coalescence event GW190814 is a hypernuclear star. We use density functional …

The possible signatures of the presence of hyperons inside neutron stars are discussed
within a Bayesian inference framework applied to a set of models based on a density …

Using as references the posterior probability distribution functions of the equation of state
(EOS) parameters inferred from the radii of canonical neutron stars (NSs) reported by the …

Within the covariant density functional theory of hypernuclear matter we build a series of
equations of state for hypernuclear compact stars, by calibrating the coupling constants of …

We analyze the effects of including Δ (1232) isobars in an equation of state (EoS) for cold, β-
stable neutron star (NS) matter, employing relativistic nuclear mean field theory. The …