In this Letter, we report a realistic calculation of the magnetic field profile for the equation of
state inside strongly magnetized neutron stars. Unlike previous estimates, which are widely …

Using an axisymmetric numerical code, we perform an extensive study of the magnetic-field
configurations in nonrotating neutron stars, varying the mass, magnetic-field strength and …

In this work, we investigate anisotropic effects on the equations of state (EoS) used to
describe neutron and quark stars in the framework of Rastall–Rainbow gravity. All our …

We derive an equation of state (EOS) for magnetized charge-neutral nuclear matter relevant
for a neutron star (NS). The calculations are performed within an effective chiral model …

Motivated by the recent gravitational wave detection by the LIGO–VIRGO observatories, we
study the Love number and dimensionless tidal polarizability of highly magnetized stars. We …

The densities in the cores of the neutron stars (NSs) can reach several times that of the
nuclear saturation density. The exact nature of matter at these densities is still virtually …

The aim of the present work is to investigate the effects of strong magnetic fields on the
hadron-quark phase transition point at zero temperature. To describe the hadronic phase, a …

We study the effects of the first nontrivial hexaquark, d*(2380), on the equation of state of
dense neutron star matter and investigate the consequences of its existence for neutron …

In this work, we explore different aspects in which strong magnetic fields play a role in the
composition, structure and evolution of neutron stars. More specifically, we discuss (i) how …

We investigate the properties of equation of state, the quark fraction, the isospin chemical
potential, and the entropy per baryon of strange quark matter at finite temperature under …