Exact Dissipative Cosmologies with Stiff Fluid

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dc.creatorMak, M. K.
dc.creatorHarko, T.
dc.date2001-07-02
dc.date.accessioned2026-07-07T11:29:54Z
dc.date.available2026-07-07T11:29:54Z
dc.descriptionThe 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.
dc.description7 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0107004
dc.identifierhttp://arxiv.org/abs/gr-qc/0107004
dc.identifierEurophys.Lett.56:762-767,2001
dc.identifierdoi:10.1209/epl/i2001-00114-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196863
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExact Dissipative Cosmologies with Stiff Fluid
dc.typetext

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