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

C. Nonaka; N. Sasaki; S. Muroya; O. Miyamura

doi:10.1016/s0375-9474(99)85039-8

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

C. Nonaka·N. Sasaki·S. Muroya·O. Miyamura

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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.

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C. Nonaka, N. Sasaki, S. Muroya, O. Miyamura. 1999-07-12. Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model. https://doi.org/10.1016/s0375-9474(99)85039-8

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