Dissipative fluids out of hydrostatic equilibrium

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dc.creatorHerrera, L.
dc.creatorMartinez, J.
dc.date1997-10-21
dc.date.accessioned2026-07-07T11:34:23Z
dc.date.available2026-07-07T11:34:23Z
dc.descriptionIn the context of the Müller-Israel-Stewart second order phenomenological theory for dissipative fluids, we analyze the effects of thermal conduction and viscosity in a relativistic fluid, just after its departure from hydrostatic equilibrium, on a time scale of the order of relaxation times. Stability and causality conditions are contrasted with conditions for which the ''effective inertial mass'' vanishes.
dc.description21 pages, 1 postscript figure (LaTex 2.09 and epsfig.sty required) Submitted to Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/gr-qc/9710099
dc.identifierhttp://arxiv.org/abs/gr-qc/9710099
dc.identifierClass.Quant.Grav.15:407-420,1998
dc.identifierdoi:10.1088/0264-9381/15/2/014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198230
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDissipative fluids out of hydrostatic equilibrium
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