Radiating Shear-Free Gravitational Collapse with Charge

Abstract

We present a new shear free model for the gravitational collapse of a spherically symmetric charged body. We propose a dissipative contraction with radiation emitted outwards. The Einstein field equations, using the junction conditions and an ansatz, are integrated numerically. A check of the energy conditions is also performed. We obtain that the charge delays the black hole formation and it can even halt the collapse.

22 pages, 9 figures. It has been corrected several typos and included several references. Accepted for publication in GRG

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Cited by in corpus (13)

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• Equilibrium, radial stability and non-adiabatic gravitational collapse of anisotropic neutron stars
• Cylindrical Thin-shell Wormholes in $f(R)$ gravity
• Stability and gravitational collapse of neutron stars with realistic equations of state
• Dynamics of Charged Bulk Viscous Collapsing Cylindrical Source With Heat Flux
• Collapse of a relativistic self-gravitating star with radial heat flux: Impact of anisotropic stresses
• Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows
• Charged Anisotropic Spherical Collapse in $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ Gravity
• New charged shear-free relativistic models with heat flux
• Radiating fluid sphere immersed in an anisotropic atmosphere
• Gravitational collapse of anisotropic stars
• Black hole formation in gravitational collapse and their astrophysical implications
• What makes a shear-free spherical perfect fluid be inhomogeneous with tidal effects?