The full set of equations governing the structure and the evolution of self-gravitating
spherically symmetric dissipative fluids with anisotropic stresses is written down in terms of …

The major goal of this work is to find solutions of Einstein–Maxwell field equations for
anisotropic, expansion-free, non-static, spherically distributed matter content. The analytical …

Spherically symmetric expansion-free distributions are systematically studied. The entire set
of field equations and junction conditions are presented for a general distribution of …

This paper investigates the internal structure and equation of state (EoS) of quark stars (QS)
with pressure anisotropy, incorporating recent astrophysical observations. Utilizing …

We obtain well behaved interior solutions describing hydrostatic equilibrium of anisotropic
relativistic stars in scale-dependent gravity, where Newton's constant is allowed to vary with …

We identify the factors responsible for the appearance of energy density inhomogeneities in
a self-gravitating fluid, and describe the evolution of those factors from an initially …

The Misner and Sharp approach to the study of gravitational collapse is extended to the
viscous dissipative case in both the streaming out and the diffusion approximations. The …

In this paper, we employ the Karmarkar condition to model a spherically symmetric radiating
star undergoing dissipative gravitational collapse within the framework of classical general …

In this paper we employ the Karmarkar condition (Proc Indian Acad Sci A 27: 56, 1948) to
model a spherically symmetric radiating star undergoing dissipative gravitational collapse in …

We consider extensions of Lemaitre-Tolman-Bondi (LTB) spacetimes to the dissipative case.
We have previously carried out a systematic study on LTB. This study is based on two …