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Exact Dissipative Cosmologies with Stiff Fluid

M. K. Mak·T. Harko
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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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M. K. Mak, T. Harko. 2001-07-02. Exact Dissipative Cosmologies with Stiff Fluid. https://doi.org/10.1209/epl%2Fi2001-00114-3

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