In this work we review the role of hyperons on the properties of neutron and proto-neutron
stars. In particular, we revise the so-called “hyperon puzzle”, go over some of the solutions …

Constraints set on key parameters of the nuclear matter equation of state (EoS) by the
values of the tidal deformability, inferred from GW170817, are examined by using a diverse …

In the context of the massive secondary object recently observed in the compact-star merger
GW190814, we investigate the possibility of producing massive neutron stars from a few …

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 …

Background: The microscopic composition and properties of infinite hadronic matter at a
wide range of densities and temperatures have been subjects of intense investigation for …

We investigate the implications of parity-violating electron scattering experiment on neutron
skin thickness of Ca 48 [calcium radius experiment (CREX)] and Pb 208 [lead radius …

In this work, we estimate how much bulk viscosity driven by Urca processes is likely to affect
the gravitational wave signal of a neutron star coalescence. In the late inspiral, we show that …

With the discovery of massive neutron stars such as PSR J1614-2230, the question has
arisen of whether exotic matter such as hyperons can exist in the neutron star core. We …

The high-density behavior of nuclear matter is analyzed within a relativistic mean field
description with nonlinear meson interactions. To assess the model parameters and their …

We investigate the impact of the neutron-star matter equation of state on the f-and p 1-mode
oscillations of neutron stars obtained within the Cowling approximation and linearized …