We calculate the number density, energy density, transverse pressure, longitudinal
pressure, and magnetization of an ensemble of spin one-half particles in the presence of a …

We study the effects of high magnetic fields on the particle population and equation of state
of hybrid stars using an extended hadronic and quark SU (3) non-linear realization of the …

Within a minimum model for neutron stars consisting of nucleons, electrons, and muons at β
equilibrium using about a dozen equations of state (EOS) from microscopic nuclear many …

We consider the gravitational lensing of rays emitted by a compact object (CO) within a
distribution of plasma with power-law density∝ r− h. For the simplest case of a cloud of …

We investigate the existence of possible stable strange matter and related stability windows
at finite temperature for different models that are generally applied to describe quark stars …

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 …

In this work, we study in detail the effects of many-body forces on the equation of state and
the structure of magnetic neutron stars. The stellar matter is described within a relativistic …

ABSTRACT The magnetar 1E 1547.0− 5408 exhibited outbursts in 2008 October and 2009
January. In this paper, we present in great detail the evolution of the temporal and spectral …

This paper gives an brief overview of the structure of hypothetical strange quarks stars
(quark stars, for short), which are made of absolutely stable 3-flavor strange quark matter …

New physics and models for the most compact astronomical objects-neutron/quark stars and
black holes are proposed. Under the new supersymmetric mirror models, neutron stars at …