Equation of State and Transport Coefficients of Relativistic Nuclear Matter

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dc.creatorMuronga, Azwinndini
dc.date2007-10-17
dc.date.accessioned2026-07-07T11:12:19Z
dc.date.available2026-07-07T11:12:19Z
dc.descriptionIn order to evaluate qualitatively the space-time evolution of hot and dense nuclear matter the underlying equation of state and transport coefficients must be known. In this study a specific equation of state is studied: the pion gas. The classical or standard transport coefficients, namely the bulk viscosity, shear viscsoity and thermal conductivity are devided by the relaxation times for the corresponding dissipative fluxes and then studied as functions of mass to temperature ratio.
dc.description5 pages, Strange Quark Matter 2007, Levoca, Slovakia
dc.identifierhttps://arxiv.org/abs/0710.3198
dc.identifierhttp://arxiv.org/abs/0710.3198
dc.identifierJ.Phys.G35:044073,2008
dc.identifierdoi:10.1088/0954-3899/35/4/044073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191341
dc.subjectNuclear Theory
dc.titleEquation of State and Transport Coefficients of Relativistic Nuclear Matter
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