{
  "annotation_id": "8ed2533d-054f-4d8a-b34d-9ca43cb7e5e3",
  "date_created": "2026-03-02T18:00:25.530000Z",
  "date_modified": "2026-03-02T18:00:25.530000Z",
  "file_hash": "2836b739ffcc18fc9759017b271011cc61228175bf9c6dd982fb5839d2142dd3",
  "private": false,
  "record": {
    "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"
    ],
    "categories": [
      "nucl-th"
    ],
    "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"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c0077c88-bb36-4429-9e99-abd85d241860",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}