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|Title:||Thermal evolution of the Kramer radiating star||Authors:||Govender, Megandhren
Maharaj, S. D.
Lorton, L. B.
|Keywords:||Schwarzschild solution;Gravitational collapse;Heat ﬂow||Issue Date:||Jan-2016||Publisher:||Springer Link||Source:||Govender, M. et al. 2016. Thermal evolution of the Kramer radiating star. PRAMANA - Journal of Physics. 86(1): 49-58.||Abstract:||The Kramer radiating star uses the interior Schwarzschild solution as a seed solution to generate a model of dissipative collapse. We investigate the thermal behaviour of the radiating star by employing a causal heat transport equation. The causal temperature is explicitly determined for the ﬁrst time by integrating the transport equation. We further show that the dissipation of energy to the exterior space-time renders the core more unstable than the cooler surface layers.||URI:||http://hdl.handle.net/10321/2950||ISSN:||0304-4289 (print)
|Appears in Collections:||Research Publications (Applied Sciences)|
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