Qualitative analysis of dissipative cosmologies

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dc.creatorDi Prisco, A.
dc.creatorHerrera, L.
dc.creatorIbanez, J.
dc.date2000-10-06
dc.date.accessioned2026-07-07T11:29:51Z
dc.date.available2026-07-07T11:29:51Z
dc.descriptionThe evolution of an homogeneous and isotropic dissipative fluid is analyzed using dynamical systems techniques. The dissipation is driven by bulk viscous pressure and the truncated Israel-Stewart theory is used. Although almost all solutions inflate, we show that only few of them can be considered as physical solutions since the dominant energy condition is not satisfied.
dc.description10 pages, 5 figures, RevTex. To appear in PRD
dc.identifierhttps://arxiv.org/abs/gr-qc/0010021
dc.identifierhttp://arxiv.org/abs/gr-qc/0010021
dc.identifierPhys.Rev.D63:023501,2001
dc.identifierdoi:10.1103/PhysRevD.63.023501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196849
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleQualitative analysis of dissipative cosmologies
dc.typetext

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