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 Effect of Gravitational Decoupling on Constraining the Mass and Radius for the Secondary
Component of GW190814 and Other Self-bound Strange Stars in f(Q) Gravity Theory …

The purpose of this paper is to obtain exact solutions for charged anisotropic spherically
symmetric matter configuration. For this purpose, we consider known solution for isotropic …

In this article, we have studied a cylindrically symmetric self-gravitating dynamical object via
complexity factor which is obtained through orthogonal splitting of Reimann tensor in f (R, T) …

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 work, we investigate astrophysical systems in a Newtonian regime using anisotropic
matter. For this purpose, we considered that both radial and tangential pressures satisfy a …

In this article, we have presented the anisotropic stars by taking a modified polytropic
equation of state (pr= k ρ 1+ 1/n− α, where k and α are constants) in the framework of the …

Relativistic polytropic models of charged anisotropic compact objects - IOPscience This site
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …

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 …