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 …

Many of the currently available equations of state for core-collapse supernova simulations
give large neutron star radii and do not provide large enough neutron star masses, both of …

The incompressibility (compression modulus) K 0 of infinite symmetric nuclear matter at
saturation density has become one of the major constraints on mean-field models of nuclear …

Motivated by a recent report by Biwas and Bose (Phys Rev D 99: 104002, 2019) that the
observations of GW170817 to constrain the extent of pressure anisotropy in neutron stars …

The impact of anisotropic pressure models in neutron stars (NSs) is increasing their
compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …

The critical densities and impact of forming Δ (1232) resonances in neutron stars are
investigated within an extended nonlinear relativistic mean-field (RMF) model. The critical …

Continued observation of PSR J0737-3039, the double pulsar, is expected to yield a precise
determination of its primary component's moment of inertia in the next few years. Since the …

We address the question of the role of low-energy nuclear physics data in constraining
neutron star global properties, eg, masses, radii, angular momentum, and tidal deformability …

We analyze the stellar properties of the relativistic mean-field (RMF) parametrizations shown
to be consistent with the recently studied constraints related to nuclear matter, pure neutron …

A new parameter set is generated for finite and infinite nuclear system within the effective
field theory motivated relativistic mean field (ERMF) formalism. The isovector part of the …