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The final outcome of dissipative collapse in the presence of Λ
Authors:S THIRUKKANESH  S MOOPANAR  M GOVENDER
Institution:1. Department of Mathematics, Eastern University, Chenkalady, Sri Lanka
2. Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Private Bag X54001, Durban, 4000, South Africa
Abstract:We investigate the role played by the cosmological constant during gravitational collapse of a radiating star with vanishing Weyl stresses in the interior. We highlight the role played by the cosmological constant during the latter stages of collapse. The evolution of the temperature of the collapsing body is studied by employing causal heat transport equation. We show that the inclusion of the cosmological constant enhances the temperature within the stellar core.
Keywords:
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