Gravitational collapse in spatially isotropic coordinates
dc.contributor.author | Govender, Megandhren | en_US |
dc.contributor.author | Bogadi, Robert | en_US |
dc.contributor.author | Sharma, Ranjan | en_US |
dc.contributor.author | Das, Shyam | en_US |
dc.date.accessioned | 2018-04-10T06:49:46Z | |
dc.date.available | 2018-04-10T06:49:46Z | |
dc.date.issued | 2015-01-21 | |
dc.description.abstract | We 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.description.availability | Copyright: 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. https://doi.org/10.1007/s10509-015-2616-9 | en_US |
dc.dut-rims.pubnum | DUT-005784 | en_US |
dc.format.extent | 7 p | en_US |
dc.identifier.citation | Govender, M. et al. 2015. Gravitational collapse in spatially isotropic coordinates. Atrophysics and Space Science. 361(33). https://doi.org/10.1007/s10509-015-2616-9 | en_US |
dc.identifier.doi | https://doi.org/10.1007/s10509-015-2616-9 | |
dc.identifier.issn | 0004-640X (print) | |
dc.identifier.issn | 1572-946X (online) | |
dc.identifier.uri | http://hdl.handle.net/10321/2949 | |
dc.language.iso | en | en_US |
dc.publisher | Springer Netherlands | en_US |
dc.publisher.uri | https://link.springer.com/content/pdf/10.1007%2Fs10509-015-2616-9.pdf | en_US |
dc.relation.ispartof | Astrophysics and space science (Online) | en_US |
dc.subject | Gravitational collapse | en_US |
dc.subject | Exact solutions | en_US |
dc.subject | Einstein’s field equations | en_US |
dc.subject | Radiating star model | en_US |
dc.subject | Extended irreversible thermodynamics | en_US |
dc.title | Gravitational collapse in spatially isotropic coordinates | en_US |
dc.type | Article | en_US |
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