Please use this identifier to cite or link to this item: http://hdl.handle.net/10321/2950
Title: Thermal evolution of the Kramer radiating star
Authors: Govender, Megandhren 
Maharaj, S. D. 
Mkhize, L 
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)
0973-7111 (online)
Appears in Collections:Research Publications (Applied Sciences)

Show full item record

Page view(s)

178
checked on Aug 16, 2018

Google ScholarTM

Check


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.