Abstract
AbstractIn this paper we study the shear free spherical symmetric gravitational collapse of a charged radiating star. All the physical quantities including pressure, density are regular. Energy conditions are satisfied throughout the interior of the matter configuration. The luminosity is time independent and mass is radiated linearly. The causal and non causal temperature remain greater than that of the uncharged collapsing scenario.
Funder
Board of Research in Nuclear Sciences
Department of Science and Technology, Ministry of Science and Technology, India
Publisher
Springer Science and Business Media LLC
Reference61 articles.
1. J.R. Oppenheimer, H. Snyder, Phys. Rev. 56, 455 (1939)
2. S. Datt, Zs. f. Phys. 108, 314 (1938)
3. S.W. Hawking, G.R. Ellis, The Large Scale Structure of Spacetime (Cambridge University Press, Cambridge, 1975)
4. P.S. Joshi, Gravitational Collapse and Spacetime Singularities (Cambridge University Press, Cambridge, 2007)
5. A.K.G. de Oliveira, N.O. Santos, C.A. Kolassis, Mon. Not. R. Astron. Soc. 216, 1001 (1985)
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