Context. An equation of state (EoS) of dense nuclear matter is a prerequisite for studies of
the structure and evolution of compact stars. A unified EoS should describe the crust and the …

Analytical representations are derived for two equations of state (EOSs) of neutron-star
matter: FPS and SLy. Each of these EOSs is unified, that is, it describes the crust and the …

Aims. In this paper, we study the global properties of neutron stars (NSs), as predicted by the
Brussels-Montreal equations of state (EoSs). These EoSs, which provide a unified …

We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the
core based on modern microscopic calculations using the Argonne v 18 potential plus three …

The theory of the nuclear energy-density functional is used to provide a unified and
thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …

Background: Recent observational data on neutron star masses and radii provide stringent
constraints on the equation of state of neutron rich matter [Annu. Rev. Nucl. Part. Sci. 62, 485 …

We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …

The transition density ρ t and pressure P t at the inner edge separating the liquid core from
the solid crust of neutron stars are systematically studied using a modified Gogny (MDI) and …

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 …

Neutron star radii provide useful information about the equation of state of neutron-rich
matter. Particularly interesting is the density dependence of the equation of state (EOS). For …