We investigate the conditions for the (in) stability of the isotropic pressure condition in
collapsing spherically symmetric, dissipative fluid distributions. It is found that dissipative …

The main objective of this work, is to develop a novel general framework for generating
solutions of stellar models in f (R) theory of gravity with class one metric. Such framework is …

The motivation of this paper is based on the foundation of extended teleparallel gravity with
matter coupling to prospect the accelerated expansion of the Universe. This theory based on …

In this work we study class I interior solutions supported by anisotropic polytropes. The
generalized Lane–Emden equation compatible with the embedding condition is obtained …

In this work we propose a novel approach to integrate the Lane–Emden equations for
relativistic anisotropic polytropes. We take advantage of the fact that Gravitational …

We generate the Einstein–Gauss–Bonnet field equations in higher dimensions for a
spherically symmetric static spacetime. The matter distribution is a neutral fluid with isotropic …

The aim of the present paper is to find an exact anisotropic and charged version of the well-
known Heintzmann interior solution [Z. Phys. 228 (1969) 489] in a space-time via the …

We model anisotropic compact stars by solving Einstein field equation with a generalized
form of equation of state (EoS) and a physically reasonable metric potential g_ rr g rr which …

In this paper, we investigate the influence of tidal Love numbers on the equation-of-state
(EoS) governing the interior matter distribution of a compact star within the framework of …

It is shown that the expressions for the tangential pressure, the anisotropy factor and the
radial pressure in the Einstein–Maxwell equations may serve as generating functions for …