{
  "id": "nucl-th/0205040",
  "version": "v3",
  "published": "2002-05-15T08:16:23.000Z",
  "updated": "2002-09-24T05:05:07.000Z",
  "title": "Comparison of space-time evolutions of hot/dense matter in $\\sqrt{s_{NN}}$=17 and 130 GeV relativistic heavy ion collisions based on a hydrodynamical model",
  "authors": [
    "Kenji Morita",
    "Shin Muroya",
    "Chiho Nonaka",
    "Tetsufumi Hirano"
  ],
  "comment": "28 pages, 21 figures, REVTeX4, one figure is added and some figures are replaced",
  "journal": "Phys.Rev. C66 (2002) 054904",
  "doi": "10.1103/PhysRevC.66.054904",
  "categories": [
    "nucl-th",
    "hep-ph"
  ],
  "abstract": "Based on a hydrodynamical model, we compare 130 GeV/$A$ Au+Au collisions at RHIC and 17 GeV/$A$ Pb+Pb collisions at SPS. The model well reproduces the single-particle distributions of both RHIC and SPS. The numerical solution indicates that huge amount of collision energy in RHIC is mainly used to produce a large extent of hot fluid rather than to make a high temperature matter; longitudinal extent of the hot fluid in RHIC is much larger than that of SPS and initial energy density of the fluid is only 5% higher than the one in SPS. The solution well describes the HBT radii at SPS energy but shows some deviations from the ones at RHIC.",
  "revisions": [
    {
      "version": "v3",
      "updated": "2002-09-24T05:05:07.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "24.10.Nz",
      "25.75.Gz",
      "12.38.Mh"
    ],
    "keywords": [
      "gev relativistic heavy ion collisions",
      "hydrodynamical model",
      "hot/dense matter",
      "space-time evolutions",
      "comparison"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Phys. Rev. C"
    },
    "note": {
      "typesetting": "RevTeX",
      "pages": 28,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 586890
    }
  }
}