{
  "annotation_id": "e1772d69-7a1d-4e65-a997-aad262b46d18",
  "date_created": "2026-03-02T18:00:07.828000Z",
  "date_modified": "2026-03-02T18:00:07.828000Z",
  "file_hash": "21821f8b3b49740f6d33f3753ec96006572e4e70df5ae03df7d5f2a5befb5629",
  "private": false,
  "record": {
    "abstract": "An effective computer program for three dimensional relativistic\nhydrodynamical model has been developed. It implements a new approach to the\nearly hot phase of relativistic heavy-ion collisions. The computer program\nsimulates time-space evolution of nuclear matter in terms of ideal-fluid\ndynamics. Equations of motions of hydrodynamics are solved making use of finite\ndifference methods. Commonly-used algorithms of numerical relativistic\nhydrodynamics RHLLE and MUSTA-FORCE have been applied in simulations. To\nspeed-up calculations, parallel processing has been made available for solving\nhydrodynamical equations. The test results of simulations for 3D, 2D and\nBjorken expansion are reported in this paper. As a next step we plan to\nimplement the hadronization algorithm by implementing the continuous particle\nemission for freeze-out and comparing it with Cooper-Frye formula.",
    "arxiv_id": "nucl-th/0601095",
    "authors": [
      "Daniel Kikola",
      "Wiktor Peryt",
      "Yuri M. Sinyukov",
      "Marcin Slodkowski",
      "Marek Szuba"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1556/APH.27.2006.2-3.43",
    "journal_ref": "Acta Phys.Hung. A27 (2006) 373-378",
    "title": "The new computer program for three dimensional relativistic   hydrodynamical model",
    "url": "https://arxiv.org/abs/nucl-th/0601095"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "9499022a-5f15-414c-9af8-bb39aae672ce",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}