{
  "annotation_id": "749476f0-eda4-4e3d-b51b-015c20f5af06",
  "date_created": "2026-03-02T18:00:19.145000Z",
  "date_modified": "2026-03-02T18:00:19.145000Z",
  "file_hash": "56977281e47ed050a9f7cb92096edd464b1123227f6924000b8d0ecc7f7367e6",
  "private": false,
  "record": {
    "abstract": "A very intuitive description of nucleus-nucleus collision phenomena is\nprovided by the relativistic fluid dynamics. We consider a 1+1 dimensional\nrelativistic imperfect fluid flow to approximate the high energy heavy ion\ncollision. The article investigates the application of the continuous symmetry\ngroup on the relativistic fluid energy-momentum tensor conservation equations\nin the ultrarelativistic limit $\\gamma \\rightarrow \\infty$.",
    "arxiv_id": "nucl-th/9609060",
    "authors": [
      "C Alexa",
      "D Vrinceanu"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "On the symmetries of the 1+1 dimensional relativistic fluid dynamics",
    "url": "https://arxiv.org/abs/nucl-th/9609060"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f3e68f1e-ab32-4890-8f2d-937660198935",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}