{
  "annotation_id": "3a7665be-55c3-4301-a6cd-2c5bdd0f1cb1",
  "date_created": "2026-03-02T18:00:04.754000Z",
  "date_modified": "2026-03-02T18:00:04.754000Z",
  "file_hash": "431fced03d4cef38f524f6d766beec1e4dd1d9559737034a44d8e5ec4cfdbeaf",
  "private": false,
  "record": {
    "abstract": "Explicit equations are given for describing the space-time evolution of\nnon-ideal (viscous) relativistic fluids undergoing boost-invariant longitudinal\nand arbitrary transverse expansion. The equations are derived from the\nsecond-order Israel-Stewart approach which ensures causal evolution. Both\nazimuthally symmetric (1+1)-dimensional and non-symmetric (2+1)-dimensional\ntransverse expansion are discussed. The latter provides the formal basis for\nthe hydrodynamic computation of elliptic flow in relativistic heavy-ion\ncollisions including dissipative effects.",
    "arxiv_id": "nucl-th/0510014",
    "authors": [
      "Ulrich W. Heinz",
      "Huichao Song",
      "Asis K. Chaudhuri"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.73.034904",
    "journal_ref": "Phys.Rev.C73:034904,2006",
    "title": "Dissipative hydrodynamics for viscous relativistic fluids",
    "url": "https://arxiv.org/abs/nucl-th/0510014"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "2f76d93d-bb81-4b2f-9332-f071ebba677f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}