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dc.contributor.authorGovender, Megandhren-
dc.contributor.authorBogadi, Robert-
dc.contributor.authorSharma, Ranjan-
dc.contributor.authorDas, Shyam-
dc.identifier.citationGovender, M. et al. 2015. Gravitational collapse in spatially isotropic coordinates. Atrophysics and Space Science. 361(33).
dc.identifier.issn0004-640X (print)-
dc.identifier.issn1572-946X (online)-
dc.description.abstractWe investigate the dynamical nature of the col-lapse process of a spherically symmetric star undergoing dissipative collapse. The star collapses from an initial static configuration by dissipating energy in the form of a radial heat flux. The perturbation in the density and pressure pro-files are such that the star is always close to hydrostatic equi-librium. The temperature profiles are studied using a causal heat transport equation.en_US
dc.format.extent7 pen_US
dc.publisherSpringer Netherlandsen_US
dc.subjectGravitational collapseen_US
dc.subjectExact solutionsen_US
dc.subjectEinstein’s field equationsen_US
dc.subjectRadiating star modelen_US
dc.subjectExtended irreversible thermodynamicsen_US
dc.titleGravitational collapse in spatially isotropic coordinatesen_US
dc.description.availabilityCopyright: 2015. Springer Netherlands. 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 Atrophysics and Space Science, Vol 361, No. 33.
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Appears in Collections:Research Publications (Applied Sciences)
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