{
  "annotation_id": "95255ef2-4700-4ada-a6d4-6310036d0aac",
  "date_created": "2026-03-02T18:00:18.948000Z",
  "date_modified": "2026-03-02T18:00:18.948000Z",
  "file_hash": "2c0988cce596d134f459a40cc37da3558e0047ceaea83d95a28f4c96f4f5094d",
  "private": false,
  "record": {
    "abstract": "The sigma-omega model in mean-field approximation where the meson fields are\ntreated classically, describes much of observed nuclear structure and has been\nemployed to describe the nuclear equation of state up to the quark-gluon phase\ntransition. The acceleration of the meson sources, for example, in relativistic\nheavy-ion collisions, should result in bremsstrahlung-like radiation of the\nmeson fields. The many mesons emitted serve to justify the use of classical\nmeson fields. The slowing of the nuclei during the collision is modeled here as\na smooth transition from initial to final velocity. Under ultra-relativistic\nconditions, vector radiation dominates. The angular distribution of energy flux\nshows a characteristic shape. It appears that if the vector meson field couples\nto the conserved baryon current, independent of the baryonic degrees of\nfreedom, this mechanism will contribute to the radiation seen in relativistic\nheavy-ion collisions. The possible influence of the quark-gluon plasma is also\nconsidered.",
    "arxiv_id": "nucl-th/9610021",
    "authors": [
      "Bryan E. Barmore"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/S0375-9474(97)80702-6",
    "journal_ref": "Nucl.Phys. A622 (1997) 605-619",
    "title": "Vector meson radiation in relativistic heavy-ion collisions",
    "url": "https://arxiv.org/abs/nucl-th/9610021"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "ee66b244-d30a-4cbd-9f95-2681d32b8c53",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}