dorsal/arxiv
View SchemaAnalyses of collective flow and space-time evolution based on relativistic hydrodynamical model
| Authors | C. Nonaka, N. Sasaki, S. Muroya, O. Miyamura |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9907046 |
| URL | https://arxiv.org/abs/nucl-th/9907046 |
| DOI | 10.1016/S0375-9474(99)85039-8 |
| Journal | Nucl.Phys.A661:353-356,1999 |
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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"abstract": "We numerically solve fully (3+1)-dimensional relativistic hydrodynamical\nequation with the baryon number conservation law. For realistic initial\nconditions we adopt the results from the event generator (URASiMA). Using this\nmodel we discuss collective flow.",
"arxiv_id": "nucl-th/9907046",
"authors": [
"C. Nonaka",
"N. Sasaki",
"S. Muroya",
"O. Miyamura"
],
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],
"doi": "10.1016/S0375-9474(99)85039-8",
"journal_ref": "Nucl.Phys.A661:353-356,1999",
"title": "Analyses of collective flow and space-time evolution based on relativistic hydrodynamical model",
"url": "https://arxiv.org/abs/nucl-th/9907046"
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