Three dimensional relativistic hydrodynamical model for QGP gas

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dc.creatorNonaka, C.
dc.creatorMuroya, S.
dc.creatorMiyamura, O.
dc.date1999-07-12
dc.date.accessioned2026-07-07T05:43:11Z
dc.date.available2026-07-07T05:43:11Z
dc.descriptionWe numerically solve fully (3+1)-dimensional relativistic hydrodynamical equation coupled with the baryon number conservation law without spatial symmetry. We discuss the effect of transverse expansion based on the deviation our numerical result from Bjorken's scaling solution. We analyze the space-time evolution of the QGP gas in the case of non cylindrical initial conditions.
dc.description5 pages, 9 figures, LaTeX2e, Talk presented at First Symposium on Science of Hadrons under Extreme Conditions, JAERI, March 11-12, 1999
dc.identifierhttps://arxiv.org/abs/nucl-th/9907045
dc.identifierhttp://arxiv.org/abs/nucl-th/9907045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/83213
dc.subjectNuclear Theory
dc.titleThree dimensional relativistic hydrodynamical model for QGP gas
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