Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
1996-02-23
J.Math.Phys.37:2906-2919,1996
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
RevTeX file, 23 pages. Accepted for publication in J. Math. Phys
Scientific paper
10.1063/1.531546
The Einstein's field equations of Friedmann-Robertson-Walker universes filled with a dissipative fluid described by both the {\em truncated} and {\em non-truncated} causal transport equations are analyzed using techniques from dynamical systems theory. The equations of state, as well as the phase space, are different from those used in the recent literature. In the de Sitter expansion both the hydrodynamic approximation and the non-thermalizing condition can be fulfilled simultaneously. For $\Lambda=0$ these expansions turn out to be stable provided a certain parameter of the fluid is lower than 1/2. The more general case $\Lambda>0$ is studied in detail as well.
Mendez Vicenc
Triginer Josep
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