Bianchi Type I Universes with Causal Bulk Viscous Cosmological Fluid

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dc.creatorMak, M. K.
dc.creatorHarko, T.
dc.date2001-10-15
dc.date.accessioned2026-07-07T11:29:54Z
dc.date.available2026-07-07T11:29:54Z
dc.descriptionWe consider the dynamics of a causal bulk viscous cosmological fluid filled constantly decelerating Bianchi type I space-time. The matter component of the Universe is assumed to satisfy a linear barotropic equation of state and the state equation of the small temperature Boltzmann gas. The resulting cosmological models satisfy the condition of smallness of the viscous stress. The time evolution of the relaxation time, temperature, bulk viscosity coefficient and comoving entropy of the dissipative fluid is also obtained.
dc.description11 pages, 5 figures, accepted for publication in International Journal of Modern Physics D
dc.identifierhttps://arxiv.org/abs/gr-qc/0110069
dc.identifierhttp://arxiv.org/abs/gr-qc/0110069
dc.identifierInt.J.Mod.Phys.D11:447-462,2002
dc.identifierdoi:10.1142/S0218271802001743
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196865
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBianchi Type I Universes with Causal Bulk Viscous Cosmological Fluid
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