Spherically symmetric cosmological solutions.
This thesis examines the role of shear in inhomogeneous spherically symmetric spacetimes in the field of general relativity. The Einstein field equations are derived for a perfect fluid source in comoving coordinates. By assuming a barotropic equation of state, two classes of nonaccelerating solutio...
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| Language: | en |
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2012
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| Online Access: | http://hdl.handle.net/10413/4842 |