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Spherically symmetric dissipative anisotropic fluids: A general study

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arxiv gr-qc/0403006 v1 pith:O4Y5Z5Q6 submitted 2004-02-29 gr-qc astro-ph

classification gr-qcastro-ph
keywords generalanisotropicdensitydissipativefluidssphericallysymmetrictensor
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The full set of equations governing the evolution of self--gravitating spherically symmetric dissipative fluids with anisotropic stresses is deployed and used to carry out a general study on the behaviour of such systems, in the context of general relativity. Emphasis is given to the link between the Weyl tensor, the shear tensor, the anisotropy of the pressure and the density inhomogeneity. In particular we provide the general, necessary and sufficient, condition for the vanishing of the spatial gradients of energy density, which in turn suggests a possible definition of a gravitational arrow of time. Some solutions are also exhibited to illustrate the discussion.

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Cited by 2 Pith papers

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    gr-qc 2024-11 conditional novelty 5.0 of 10

    Tidal heating imprints from black hole horizons can be captured by two effective parameters and modeled through merger, offering a future test to distinguish black holes from exotic horizonless objects.

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