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 …

This review aims at providing an extensive discussion of modern constraints relevant for
dense and hot strongly interacting matter. It includes theoretical first-principle results from …

The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with
Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the …

One of the most common assumptions has been made that the pressure inside the star is
isotropic in nature. However, the pressure is locally anisotropic in nature which is a more …

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which
seeks to understand the nuclear engines of astronomical objects and the origin of the …

It is widely believed that the binary neutron star merger GW190425 produced a black hole
promptly upon merger. Motivated by the potential association with the fast radio burst FRB …

Astrophysical observations of neutron stars have been widely used to infer the properties of
the nuclear matter equation of state. Beside being a source of information on average …

We investigate the nuclear symmetry energy and neutron star properties using a Bayesian
analysis based on constraints from different chiral effective field theory calculations using …

We systematically study the properties of pure nucleonic and hyperonic magnetic stars using
a density-dependent relativistic mean-field (DD-RMF) equations of state. We explore several …

In this work we investigate the minimal physical requirements needed for generating a
speed of sound that surpasses its asymptotic conformal limit. It is shown that a peak in the …