In this article we study the hydrostatic equilibrium configuration of neutron stars and strange
stars, whose fluid pressure is computed from the equations of state p= ωρ 5/3 and p= 0.28 …

We present a simple and effective new methodology to build up self-gravitating structures
driven by an imperfect fluid distributions. This approach is developed within the framework of …

In this work we study the properties of compact spheres made of a charged perfect fluid with
a MIT bag model EoS for quark matter. Considering static spherically symmetric spacetime …

We study radial oscillations of hybrid nonrotating neutron stars composed by a quark matter
core and hadronic external layers. At first, we physically deduce the junction conditions that …

In this current study, our main focus is on modeling the specific charged compact star SAX J
1808.4-3658 (M= 0.88 M_ ⊙ M⊙, R= 8.9 km) within the framework of f (R,\, T) f (R, T) …

In the present work, we investigate the effects of dark matter (DM) on hybrid star properties.
We assume that dark matter is mixed with both hadronic and quark matter and interacts with …

We have investigated the possibility of existing a class of compact charged spheres made of
a charged perfect fluid in the context of recently proposed 4 D Einstein–Gauss–Bonnet …

We investigate the effects of the modified f (R, T) gravity on the charged strange quark stars
with the standard choice of f (R, T)= R+ 2χ T. Those types of stars are supposed to be made …

This work analyses the hydrostatic equilibrium configurations of strange stars in a non-
minimal geometry-matter coupling (GMC) theory of gravity. Those stars are made of strange …

The present article discusses a charged spherical solution in modified f (G, T) gravity under
the embedding class I condition, where f (G, T)= G 2+ χ T, where G is a Gauss–Bonnet term …