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Exact Dissipative Cosmologies with Stiff Fluid

2001/07/02 by M. K. Mak, T. Harko · 1 citation
Physics and Astronomy · #gr-qc

paper · pdf · doi:10.1209/epl/i2001-00114-3

published as Europhys.Lett.56:762-767,2001 · 7 pages, 6 figures

arxiv created 2001/07/02 · arxiv updated 2009/11/30

Abstract

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.

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