Relativistic Dynamics of Non-ideal Fluids: Viscous and heat-conducting fluids I. General Aspects and 3+1 Formulation for Nuclear Collisions

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dc.creatorMuronga, Azwinndini
dc.date2006-11-25
dc.date2007-07-31
dc.date.accessioned2026-07-07T11:23:55Z
dc.date.available2026-07-07T11:23:55Z
dc.descriptionRelativistic non-ideal fluid dynamics is formulated in 3+1 space--time dimensions. The equations governing dissipative relativistic hydrodynamics are given in terms of the time and the 3-space quantities which correspond to those familiar from non-relativistic physics. Dissipation is accounted for by applying the causal theory of relativistic dissipative fluid dynamics. As a special case we consider a fluid without viscous/heat couplings in the causal system of transport/relaxation equations. For the study of physical systems we consider pure (1+1)-dimensional expansion in planar geometry, (1+1)-dimensional spherically symmetric ({\em fireball}) expansion, (1+1)-dimensional cylindrically symmetric expansion and a (2+1)-dimensional expansion with cylindrical symmetry in the transverse plane ({\em firebarell} expansion). The transport/relaxation equations are given in terms of the spatial components of the dissipative fluxes, since these are not independent. The choice for the independent components is analogous to the non-relativistic equations.
dc.description49 pages, added references, typos added
dc.identifierhttps://arxiv.org/abs/nucl-th/0611090
dc.identifierhttp://arxiv.org/abs/nucl-th/0611090
dc.identifierPhys.Rev.C76:014909,2007
dc.identifierdoi:10.1103/PhysRevC.76.014909
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195054
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleRelativistic Dynamics of Non-ideal Fluids: Viscous and heat-conducting fluids I. General Aspects and 3+1 Formulation for Nuclear Collisions
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