Exact Dissipative Cosmologies with Stiff Fluid
arXiv:gr-qc/0107004 · doi:10.1209/epl/i2001-00114-3
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.
7 pages, 6 figures
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