Qualitative Analysis of Causal Cosmological Models

dc.creatorMendez, Vicenç
dc.creatorTriginer, Josep
dc.date1996-02-23
dc.date.accessioned2026-07-07T11:34:21Z
dc.date.available2026-07-07T11:34:21Z
dc.descriptionThe 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 $Λ=0$ these expansions turn out to be stable provided a certain parameter of the fluid is lower than 1/2. The more general case $Λ>0$ is studied in detail as well.
dc.descriptionRevTeX file, 23 pages. Accepted for publication in J. Math. Phys
dc.identifierhttps://arxiv.org/abs/gr-qc/9602044
dc.identifierhttp://arxiv.org/abs/gr-qc/9602044
dc.identifierJ.Math.Phys.37:2906-2919,1996
dc.identifierdoi:10.1063/1.531546
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198220
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQualitative Analysis of Causal Cosmological Models
dc.typetext

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