http://arxiv.org/abs/1506.02422
We review a recently proposed framework for studying axially symmetric dissipative fluids \cite{Ref1}. Some general results are discussed at the most general level. We then proceed to analyze some particular cases. First, the shear-free case is considered \cite{3}. We shall next discuss the perfect fluid case under the geodesic condition, without impossing ab initio the shear–free condition \cite{2}. Finally a dissipative, geodesic fluid \cite{4}, is analyzed in some detail. We conclude by bringing out the attention to some open issues.
L. Herrera
Wed, 10 Jun 15
38/53
Comments: Talk given at the International Conference on Relativistic Astrophysics (through Skype), Lahore, February 2015. To appear in the proceedings, to be published by Punjab University Press. 9 pages, Revtex-4
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