{
  "annotation_id": "933d8550-f04d-44ae-83c4-c565ec7f4ada",
  "date_created": "2026-03-02T18:00:15.487000Z",
  "date_modified": "2026-03-02T18:00:15.487000Z",
  "file_hash": "3ddc77a33180048b8ae537a9294f25cea3a1a01507e2dc98e2a0182f9eb049f6",
  "private": false,
  "record": {
    "abstract": "The influence of the dissipative terms on the conditions of formation and the\ncharacteristic parameters of shock waves in relativistic nuclear collisions is\ninvestigated for three types of equation of state (non linear QHD-1, resonance\ngas and lattice QCD). Energy and velocity profiles are obtained in a\none-dimensional model; the duration of the shock phase and width of the shock\nfront are calculated. It is shown that the presence of a phase transition\nresults in a strong enhancement of the width of the shock front, which results\nin an increase of transparency. This effect, combined with the fact that the\nnuclei have a finite size, prevents the energy density to rise to its maximum\nvalue (full stopping) as would be predicted by a non dissipative shock model.",
    "arxiv_id": "nucl-th/9412012",
    "authors": [
      "L. Mornas",
      "U. Ornik"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0375-9474(95)00036-Z",
    "journal_ref": "Nucl.Phys. A587 (1995) 828-852",
    "title": "On the Role of Dissipation in the Early Stages of Relativistic Heavy Ion   Collisions",
    "url": "https://arxiv.org/abs/nucl-th/9412012"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "38d92450-c955-4534-9b55-a694a5ad3e0b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}