Junction Conditions and Consequences of Quasi-Spherical Space-Time with Electro-Magnetic Field and Vaidya Matric

Abstract

In this work the junction conditions between the exterior Reissner-Nordstrom-Vaidya space-time with the interior quasi-spherical Szekeres space-time have been studied for analyzing gravitational collapse in the presence of a magneto-hydrodynamic fluid undergoing dissipation in the form of heat flow. We have discussed about the apparent horizon and have evaluated the time difference between the formation of apparent horizon and central singularity.

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References in corpus (3)

• Quasi-spherical collapse with cosmological constant
• Non-adiabatic collapse of a quasi-spherical radiating star
• Role of Pressure in Quasi-Spherical Gravitational Collapse

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• Dynamics of Charged Plane Symmetric Gravitational Collapse
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• Gravitational Charged Perfect Fluid Collapse in Friedmann Universe Models
• Dynamics of Viscous Dissipative Plane Symmetric Gravitational Collapse
• Influence of $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ Gravity on Cylindrical Collapse
• Study of Charged Cylindrical Collapse in $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ Gravity
• Charged Anisotropic Spherical Collapse in $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ Gravity
• Gravitational Perfect Fluid Collapse in Gauss-Bonnet Gravity