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 progress in theoretical modeling of compact high-mass stars in the context of alternative
gravity has become important in minimizing challenges associated with neutron star (NS) …

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 construct a unique anisotropic solution for spherically symmetric spacetime
by investigating the Chaplygin EOS for the anisotropic fluid distribution. For generating the …

The current paper presents a double-layered neutral anisotropic stellar model in general
relativistic setting. The model is developed by using Einstein field equations and class I …

This paper investigates a spherically symmetric compact relativistic body with isotropic
pressure profiles within the framework of general relativity. In order to solve the Einstein's …

In this paper, we analyse an analytical solution of the Einstein–Maxwell field equations that
considers matter with anisotropic pressures in a static and spherically symmetric geometry …

In this work, we present a class of relativistic and well-behaved solution to the Einstein's field
equations for anisotropic matter distribution. We perform our analysis by using the Buchdahl …

In this paper, we have constructed a well-behaved, realistic and stable model for relativistic
compact star in the presence of isotropic charged fluid by solving the Einstein–Maxwell field …

By using the quadratic equation of state and the anisotropic energy-momentum tensor for
compact stars in spherically symmetric spacetime in hydrostatic static equilibrium to solve …