dorsal/arxiv
View SchemaWhat can we learn from hydrodynamic analysis at RHIC?
| Authors | Tetsufumi Hirano |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0511036 |
| URL | https://arxiv.org/abs/nucl-th/0511036 |
| DOI | 10.1016/j.nuclphysa.2006.06.025 |
| Journal | Nucl.Phys.A774:531-534,2006; Eur.Phys.J.A29:19-22,2006 |
Abstract
We can establish a new picture, the perfect fluid sQGP core and the dissipative hadronic corona, of the space-time evolution of produced matter in relativistic heavy ion collisions at RHIC. It is also shown that the picture works well also in the forward rapidity region through an analysis based on a new class of the hydro-kinetic model and that this is a manifestation of rapid increase of entropy density in the vicinity of QCD critical temperature, namely deconfinement.
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"abstract": "We can establish a new picture, the perfect fluid sQGP core and the\ndissipative hadronic corona, of the space-time evolution of produced matter in\nrelativistic heavy ion collisions at RHIC. It is also shown that the picture\nworks well also in the forward rapidity region through an analysis based on a\nnew class of the hydro-kinetic model and that this is a manifestation of rapid\nincrease of entropy density in the vicinity of QCD critical temperature, namely\ndeconfinement.",
"arxiv_id": "nucl-th/0511036",
"authors": [
"Tetsufumi Hirano"
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"doi": "10.1016/j.nuclphysa.2006.06.025",
"journal_ref": "Nucl.Phys.A774:531-534,2006; Eur.Phys.J.A29:19-22,2006",
"title": "What can we learn from hydrodynamic analysis at RHIC?",
"url": "https://arxiv.org/abs/nucl-th/0511036"
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