Radiating solutions with heat flow in general relativity.
In this thesis we model spherically symmetric radiating stars dissipating energy in the form of a radial heat flux. We assume that the spacetime for the interior matter distribution is shear-free. The junction conditions necessary for the matching of the exterior Vaidya solution to an interior radia...
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| Language: | en |
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2012
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| Online Access: | http://hdl.handle.net/10413/4836 |