Please use this identifier to cite or link to this item: http://hdl.handle.net/10321/2950
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dc.contributor.authorGovender, Megandhren-
dc.contributor.authorMaharaj, S. D.-
dc.contributor.authorMkhize, L-
dc.contributor.authorLorton, L. B.-
dc.date.accessioned2018-04-10T06:53:32Z-
dc.date.available2018-04-10T06:53:32Z-
dc.date.issued2016-01-
dc.identifier.citationGovender, M. et al. 2016. Thermal evolution of the Kramer radiating star. PRAMANA - Journal of Physics. 86(1): 49-58.en_US
dc.identifier.issn0304-4289 (print)-
dc.identifier.issn0973-7111 (online)-
dc.identifier.urihttp://hdl.handle.net/10321/2950-
dc.description.abstractThe 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.en_US
dc.format.extent10 pen_US
dc.language.isoenen_US
dc.publisherSpringer Linken_US
dc.subjectSchwarzschild solutionen_US
dc.subjectGravitational collapseen_US
dc.subjectHeat flowen_US
dc.titleThermal evolution of the Kramer radiating staren_US
dc.typeArticleen_US
dc.publisher.urihttps://link.springer.com/content/pdf/10.1007%2Fs12043-015-0967-y.pdfen_US
dc.dut-rims.pubnumDUT-005785en_US
dc.description.availabilityCopyright: 2016. Springer India. Due to copyright restrictions, only the abstract is available. For access to the full text item, please consult the publisher's website. The definitive version of the work is published in Pramana – Journal of Physics, Vol 86, No. 49. https://doi.org/10.1007/s12043-015-0967-yen_US
item.fulltextNo Fulltext-
item.grantfulltextnone-
Appears in Collections:Research Publications (Applied Sciences)
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