In the present paper we generate a set of solutions describing the interior of a compact star
under f (R, T) f (R, T) theory of gravity which admits conformal motion. An extension of …

In this work, we present a hierarchical solution-generating technique employing the
Minimum Gravitational Decoupling (MGD) Method and the generalized concept of …

In a recent approach in modeling a radiating relativistic star undergoing gravitational
collapse the role of the Weyl stresses was emphasized. It is possible to generate a model …

We study the effects of pressure anisotropy and heat dissipation in a spherically symmetric
radiating star undergoing gravitational collapse. An exact solution of the Einstein field …

This paper explores a new embedding anisotropic charged version of a solution to Einstein–
Maxwell field equations in four-dimensional spacetime through the Karmarkar conditions …

We employ a perturbative scheme to study the evolution of a spherically symmetric stellar
body undergoing gravitational collapse in the presence of heat dissipation and anisotropic …

We investigate the role played by density inhomogeneities and dissipation on the final
outcome of collapse of a self-gravitating sphere. By imposing a perturbative scheme on the …

In this paper, we have investigated the non-adiabatic spherical gravitational collapse in the
framework of the f (R, T) theory of gravity with a locally anisotropic fluid that undergoes …

The influence of an equation of state on the dynamical (in) stability of a sphere undergoing
dissipative collapse is investigated for various forms of matter distributions. Employing a …

We study the gravitational behavior of a spherically symmetric radiating star when the fluid
particles are in geodesic motion. We transform the governing equation into a simpler form …