Dissipative gravitating systems.
In this thesis we investigate the effect of shear on radiating stars undergoing gravitational collapse. The interior spacetime is described by the most general spherically symmetric line element in the absence of rotation. The energy momentum tensor for the stellar interior is taken to be an anisotr...
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| Language: | en_ZA |
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2014
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| Online Access: | http://hdl.handle.net/10413/10923 |