Collapse of a relativistic self-gravitating star with radial heat flux: Impact of anisotropic stresses

Abstract

We develop a simple model for a self-gravitating spherically symmetric relativistic star which begins to collapse from an initially static configuration by dissipating energy in the form of radial heat flow. We utilize the model to show how local anisotropy effects the collapse rate and thermal behaviour of gravitationally evolving systems.

To appear in Journal of Gravity

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Cited by in corpus (6)

• Anisotropic extension of Finch and Skea stellar model
• Radiating stars with exponential Lie symmetries
• Relativistic Polytropic Models of Charged Anisotropic Compact Object
• Charged compact stellar model in Finch-Skea spacetime
• Gravitational collapse of anisotropic stars
• Radiant gravitational collapse with anisotropy in pressures and bulk viscosity