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 discuss strange stars admixed with fermionic dark matter in the presence of a strong
magnetic field using the two-fluid Tolman-Oppenheimer-Volkov equations. We describe …

In this work a density-dependent quark model is revisited, its thermodynamic consistency
checked and the stability window for absolutely stable quark matter obtained. The …

In this paper, we investigate the evolution of strange quark stars (SQS) from birth as proto-
strange quark stars to maturity as stable SQSs at a zero temperature. We assume that self …

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 …

Based on the assumption that the QCD phase diagram gives a realistic picture of hadronic
and quark matter under different regimes, it is possible to claim that a quark core may be …

In the relativistic impulse approximation (RIA), we study symmetry potentials and in-medium
nucleon-nucleon (NN) cross sections with the Nambu–Jona-Lasinio (NJL) model that …

We investigate the hadron-quark phase transition at finite density in the presence of a
magnetic field taking into account the anisotropy created by a uniform magnetic field in the …

Using the two-fluid Tolman-Oppenheimer-Volkoff equation, the properties of dark matter
(DM) admixed neutron stars (DANSs) have been investigated. In contrast to previous …

In the context of neutron stars (NS), dense-magnetized quark and hadron models have been
well studied under the assumption that the system's pressures are isotropic. However, the …