The physical meaning of structure scalars is analyzed for charged dissipative spherical
fluids and for neutral dust in the presence of cosmological constant. The role played by such …

We present here a new shear free model for the gravitational collapse of a spherically
symmetric charged body. We propose a dissipative contraction with radiation emitted …

We consider non-adiabatic flow of the fluid possessing dissipation in the form of shearing
viscosity in electromagnetic field. The scalar functions (structure scalars) for charged plane …

This work investigates the dynamical instability of the relativistic self-gravitating collapsing
fluids with electromagnetic field in Carrol–Duvvuri–Trodden–Turner (CDTT) f (R) model for …

We derive an exact Maxwell-Einstein metric for a spherically symmetric static perfect fluid
with mass and charge (Q), that electrifies the Tolman-VII metric and meets applicable …

We investigate the evolution of non-adiabatic collapse of a shear-free spherically symmetric
stellar configuration with anisotropic stresses accompanied with radial heat flux. The …

We study the instability of cylindrically symmetric expansion-free anisotropic geometry in the
presence of electromagnetic field. For smooth matching of the interior geometry with the …

The development of dissipative and electrically charged distributions in five dimensions is
presented by using the post-quasistatic approximation. It is an iterative technique for the …

A general iterative method proposed some years ago for the description of relativistic
collapse is presented here in comoving coordinates. For doing that we redefine the basic …

This paper presents a novel class of interior solutions for anisotropic stars under the
imposition of a self-similar symmetry. This means proposing exact solutions to the Einstein …