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 crust-core (CC) phase transition of neutron stars is studied within a unified meta-
modeling of the nuclear Equation of State (EoS). The variational equations in the crust are …

The Vlasov formalism is extended to relativistic mean field hadron models with nonlinear
terms up to fourth order and applied to the calculation of the crust-core transition density …

Background: An accurate determination of the core-crust transition is necessary in the
modeling of neutron stars for astrophysical purposes. The transition is intimately related to …

In this work, we perform a Bayesian inference of the crust–core transition density ρ t of
neutron stars based on the neutron-star radius and neutron-skin thickness data using a …

Context. Few unified equations of state for neutron star matter, in which core and crust are
described using the same nuclear model, are available. However the use of non-unified …

We propose and apply a new parametrization of the modified chiral effective model to study
rotating neutron stars with hyperon cores in the framework of the relativistic mean-field …

Nuclear pasta topology is an essential ingredient to determine transport properties in the
inner crust of neutron stars. We perform semiclassical molecular dynamics simulations of …

To make best use of multifaceted astronomical and nuclear data sets, probability
distributions of neutron star models that can be used to propagate errors consistently from …

The neutron star crustal equation of state and transition point properties are computed within
a unified metamodeling approach. A Bayesian approach is employed including two types of …