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 …

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 …

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 …

In this work we investigate neutron stars (NS) in f (Script R, T) gravity for the case R+ 2λ
Script T, Script R is the Ricci scalar and Script T the trace of the energy-momentum tensor …

This paper compiles the model parameters and zero-temperature properties of an extensive
collection of published theoretical nuclear interactions, including 255 nonrelativistic (Skyrme …

The concept of quarkyonic matter presents a promising alternative to the conventional
models used to describe high-density matter and provides a more nuanced and detailed …

We present the covariance analysis of two successful nuclear energy density functionals
(EDFs),(i) a non-relativistic Skyrme functional built from a zero-range effective interaction …

The correlations of the crust-core transition density and pressure in neutron stars with the
slope of the symmetry energy and the neutron skin thickness are investigated, using different …

There are generally two factors on which the form of the symmetry energy depends. The first
one is the model involved in determining the nuclear matter equation of state, and the …