{
  "annotation_id": "06fefccf-ae30-4188-b2d2-1b23361e6534",
  "date_created": "2026-03-02T18:00:07.284000Z",
  "date_modified": "2026-03-02T18:00:07.284000Z",
  "file_hash": "8b2b5ba204c5f58d4e5ee084368aa05d8aee1412d0794e8dde83cecff6af00f9",
  "private": false,
  "record": {
    "abstract": "We study the dynamical appearance of scaling solutions in relativistic\nhydrodynamics. The phase transition effects are included through the\ntemperature dependent sound velocity. If a pre-equilibrium transverse flow is\nincluded in the initial conditions, then it may reach the form of the\nasymptotic Hubble flow, r/t, in short evolution times, 7-15 fm. The numerical\nsolutions are found to support to the freeze-out models (Blast-Wave, Buda-Lund,\nCracow).",
    "arxiv_id": "nucl-th/0510092",
    "authors": [
      "M. Chojnacki"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1556/APH.27.2006.2-3.33",
    "journal_ref": "Acta Phys.Hung. A27 (2006) 331-334",
    "title": "Hubble-like flows in relativistic heavy-ion collisions",
    "url": "https://arxiv.org/abs/nucl-th/0510092"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "df798f67-a3d7-4119-9217-74c7673b43ad",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}