Exact Dissipative Cosmologies with Stiff Fluid

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The general solution of the gravitational field equations in the flat Friedmann-Robertson-Walker geometry is obtained in the framework of the full Israel-Stewart-Hiscock theory for a bulk viscous stiff cosmological fluid, with bulk viscosity coefficient proportional to the energy density.
7 pages, 6 figures

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/196863

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0107004
 http://arxiv.org/abs/gr-qc/0107004
 Europhys.Lett.56:762-767,2001
 doi:10.1209/epl/i2001-00114-3

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arXiv