Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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4 pages, 11 figures, to apper in Proceedings of Quark Matter '99

Scientific paper

10.1016/S0375-9474(99)85039-8

We numerically solve fully (3+1)-dimensional relativistic hydrodynamical
equation with the baryon number conservation law. For realistic initial
conditions we adopt the results from the event generator (URASiMA). Using this
model we discuss collective flow.

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