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 …

In this work, we compute the structure and composition of the inner crust of a neutron star in
the presence of a strong magnetic field, such as can be found in magnetars. To determine …

In the present work, we consider nuclear matter in the innermost crust of neutron stars under
the presence of a strong magnetic field within the framework of a relativistic mean-field …

Background: The advent of new dedicated experimental programs on hyperon physics is
rapidly boosting the field, and the possibility of synthesizing multiple strange hypernuclei …

In this work, we study the effect of strong magnetic fields on the equation of state (EoS) of
warm, homogeneous, neutron star (NS) matter in beta equilibrium. NS matter is described …

We study the effect of strong magnetic fields, of the order of 10 15–10 17 G, on the extension
of the crust of magnetized neutron stars. The dynamical instability region of neutron-proton …

The effect of strong magnetic fields on the properties of the pasta structure is calculated
within a Thomas-Fermi approach using relativistic mean-field models to modulate stellar …

The effect of temperature on the crust-core transition of a magnetar is studied. The
thermodynamical spinodals are used to calculate the transition region within a relativistic …

We investigate the thermodynamic instabilities of asymmetric nuclear matter (ANM) from the
mechanical (isoscalar) and chemical (isovector) points of view in the framework of a …

The equation of state of neutron matter is affected by the presence of a magnetic field due to
the intrinsic magnetic moment of the neutron. Here we study the equilibrium configuration of …