Space-time Evolution of Quark-Gluon Plasma Fluid with First Order Phase Transition

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dc.creatorMuroya, S.
dc.creatorNonaka, C.
dc.date1997-09-05
dc.date1997-09-16
dc.date.accessioned2026-07-07T09:08:33Z
dc.date.available2026-07-07T09:08:33Z
dc.descriptionWe numerically solve the (3+1)-dimensional relativistic hydrodynamical equation with a bag-model equation of state, which is one of the simplest models for the first order phase transition. Based on the numerical solution, we discuss the space-time evolution of the hot fluid produced in ultra relativistic nuclear collisions. Especially, the space-time structure of the two-phase co-existing region during the quark-gluon plasma-hadron phase transition is analyzed in detail. Finally, we investigate the change of the mass spectra of $J/ψ$, $η_{c}$ and $ϕ$ as possible experimental signatures of the phase transition.
dc.description9 pages, latex, 7 Postscript figures
dc.identifierhttps://arxiv.org/abs/nucl-th/9709004
dc.identifierhttp://arxiv.org/abs/nucl-th/9709004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/150760
dc.subjectNuclear Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Experiment
dc.titleSpace-time Evolution of Quark-Gluon Plasma Fluid with First Order Phase Transition
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