In this review we discuss self-consistent methods to calculate the global structure of strongly
magnetised neutron stars within the general-relativistic framework. We outline why solutions …

We obtain a new equation of state for the nucleonic and hyperonic inner core of neutron
stars that fulfils the 2 M⊙ observations as well as the recent determinations of stellar radii …

The phenomenon of inverse magnetic catalysis of chiral symmetry in QCD predicted by
lattice simulations can be reproduced within the Nambu-Jona-Lasinio model if the coupling …

A neutron star was first detected as a pulsar in 1967. It is one of the most mysterious
compact objects in the universe, with a radius of the order of 10 km and masses that can …

We investigate magnetic field (e B) dependence of constituent quark mass, the longitudinal
and transverse pressure as well as the magnetization and magnetic susceptibility of strongly …

Magnetic fields are ubiquitous across different physical systems of current interest; from the
early Universe, compact astrophysical objects and heavy-ion collisions to condensed matter …

Hot QCD medium effects have been studied in the effective quasiparticle description of
quark-gluon plasma. This model encodes the collective excitation of gluons and …

We compute the pressure from first principles within perturbative QCD at finite baryon
density and very high magnetic fields up to two-loops and with physical quark masses. The …

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 …