Please use this identifier to cite or link to this item: http://hdl.handle.net/10321/2947
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dc.contributor.authorNaidu, N.F.-
dc.contributor.authorGovender, Megandhren-
dc.date.accessioned2018-04-09T07:14:45Z-
dc.date.available2018-04-09T07:14:45Z-
dc.date.issued2016-
dc.identifier.citationNaidu, N.F. and Govender, M. 2016. The influence of initial conditions during dissipative collapse. International Journal of Modern Physics D. 25(10): DOI: 10.1142/S0218271816500929en_US
dc.identifier.issn0218-2718 (print)-
dc.identifier.issn1793-6594 (online)-
dc.identifier.urihttp://hdl.handle.net/10321/2947-
dc.description.abstractStarting off with two distinct initially static stellar cores (i) Florides interior (constant density, vanishing radial pressure) and (ii) Wyman interior (constant density, nonvan-ishing radial pressure), we explore the dynamics of these two models once hydrostatic equilibrium is lost. We show that although the time of formation of horizon, evolution of the mass and proper radius are independent of the chosen initially static configurations, there is a significant difference in the temperature profiles of the radiating bodies as the collapse proceeds.en_US
dc.format.extent14 pen_US
dc.language.isoenen_US
dc.publisherWorld Scientific Publishing Companyen_US
dc.subjectHydrostatic equilibriumen_US
dc.subjectShear-free conditionen_US
dc.subjectDissipationen_US
dc.titleThe influence of initial conditions during dissipative collapseen_US
dc.typeArticleen_US
dc.dut-rims.pubnumDUT-005782en_US
item.grantfulltextopen-
item.fulltextWith Fulltext-
Appears in Collections:Research Publications (Applied Sciences)
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