Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model
Nuclear Theory
2011-04-15 v1
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.
Keywords
Cite
@article{arxiv.nucl-th/9907046,
title = {Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model},
author = {C. Nonaka and N. Sasaki and S. Muroya and O. Miyamura},
journal= {arXiv preprint arXiv:nucl-th/9907046},
year = {2011}
}
Comments
4 pages, 11 figures, to apper in Proceedings of Quark Matter '99