Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model
arXiv:nucl-th/9907046 · doi:10.1016/S0375-9474(99)85039-8
Abstract
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.
4 pages, 11 figures, to apper in Proceedings of Quark Matter '99