The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …

We discuss neutron stars with strong magnetic mean fields in the framework of Extended
Theories of Gravity. In particular, we take into account models derived from f (R) and f (Script …

We investigate the properties of anisotropic, spherically symmetric compact stars, especially
neutron stars (NSs) and strange quark stars (SQSs), made of strongly magnetized matter …

Neutron stars with strong magnetic fields are considered in the framework of f (R) gravity. In
order to describe dense matter in magnetic field, the model with baryon octet interacting …

We study the thermodynamic properties of the color-flavored-locked (CFL) quark matter in
finite temperature and strong magnetic field cases within the confined-isospin-density …

We investigate properties of strange quark matter in the framework of the SU (3) Nambu–
Jona-Lasinio model with vector interactions under strong magnetic fields. The effects of …

We study the thermodynamic properties of asymmetric quark matter and large mass quark
stars within the confined-isospin-density-dependent-quark-mass model. We find that the …

We study how the magnetic field and non-standard vector channels affect hadronic, quark
and hybrid stars. In the hadronic phase, we use the QHD model, with its standard σ ω ρ σ ω …

Within the confined isospin-and density-dependent mass model, we study the properties of
strange quark matter (SQM) and quark stars (QSs) in strong magnetic fields. The equation of …

We study the properties of strange quark matter (SQM) and quark stars (QSs) in strong
magnetic fields within the extended confined isospin-density-dependent mass (CIDDM) …