Please use this identifier to cite or link to this item:
https://hdl.handle.net/10321/2949
DC Field | Value | Language |
---|---|---|
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.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.issn | 0004-640X (print) | - |
dc.identifier.issn | 1572-946X (online) | - |
dc.identifier.uri | http://hdl.handle.net/10321/2949 | - |
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.format.extent | 7 p | en_US |
dc.language.iso | en | en_US |
dc.publisher | Springer Netherlands | 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 |
dc.publisher.uri | https://link.springer.com/content/pdf/10.1007%2Fs10509-015-2616-9.pdf | en_US |
dc.dut-rims.pubnum | DUT-005784 | 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.identifier.doi | https://doi.org/10.1007/s10509-015-2616-9 | - |
item.fulltext | No Fulltext | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.grantfulltext | none | - |
item.cerifentitytype | Publications | - |
Appears in Collections: | Research Publications (Applied Sciences) |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.