Abstract The Einstein–Maxwell (or Einstein) system of field equations plays a substantial
role in the modeling of compact stars. Although due to its non-linearity getting an exact …

The goal of this work was to investigate the behavior of charge compact stars in the context
of f (G) theory of gravity, which is one of the most powerful candidates responsible for the …

In this study, we investigate the literature on anisotropic stellar spheres in f (R, ϕ) gravity
utilizing Tolman–Kuchowicz (TK) spacetime. Due to the existence of anisotropic matter …

The Einstein-Maxwell (or Einstein) system of field equations plays a substantial role in the
modeling of compact stars. Although due to its non-linearity getting an exact solution for the …

In this paper, we amalgamate three-layer hypothesis of compact star models given by
Ginzburg (Usp Fiz Nauk 103: 393, 1971) with our recent works on core-envelope compact …

We find new classes of exact solutions to the Einstein field equations where the matter
distribution satisfies a generalized polytropic equation of state. The matter distribution is …

This manuscript is related to the construction of relativistic core-envelope model for
spherically symmetric charged anisotropic compact objects. The polytropic equation of state …

We study the dynamics of relativistic shear-free gravitating fluids in higher dimensions for
both neutral and charged matter. We reduce the Einstein–Maxwell equations to a single …

We sketch an algorithm to generate exact anisotropic solutions starting from a barotropic
EoS and setting an ansatz on the metric functions. To illustrate the method, we use a …

In this work, we present a cogent and physically well-behaved solution for neutron stars
envisaged with a core layer having quark matter satisfying the MIT-bag equation of state …