Spherically symmetric solutions in relativistic astrophysics.
In this thesis we study classes of static spherically symmetric spacetimes admitting a perfect fluid source, electromagnetic fields and anisotropic pressures. Our intention is to generate exact solutions that model the interior of dense, relativistic stars. We find a sufficient condition for the exi...
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| Language: | en |
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2011
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| Online Access: | http://hdl.handle.net/10413/3907 |