{
  "annotation_id": "60bb6c8a-960e-4342-857e-2e75160358ad",
  "date_created": "2026-03-02T18:00:04.984000Z",
  "date_modified": "2026-03-02T18:00:04.984000Z",
  "file_hash": "d80e5e30ffa8934a62365b32d77b80ec3149f4f0977fc49efc2da7ce7b455887",
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  "record": {
    "abstract": "We point out similarity of thermodynamic conditions reached in intermediate\nenergy nuclear collisions and in supernova explosions. We show that a\nstatistical approach, which has been previously applied for nuclear\nmultifragmentation reactions, can be very useful for description of\nelectro-neutral stellar matter. Then properties of hot unstable nuclei\nextracted from analysis of multifragmentation data can be used for construction\nof a realistic equation of state of supernova matter.",
    "arxiv_id": "nucl-th/0506061",
    "authors": [
      "A. S. Botvina",
      "I. N. Mishustin"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "nucl-ex"
    ],
    "doi": "10.1103/PhysRevC.72.048801",
    "journal_ref": "Phys.Rev. C72 (2005) 048801",
    "title": "Multifragmentation reactions and properties of hot stellar matter at   subnuclear densities",
    "url": "https://arxiv.org/abs/nucl-th/0506061"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7575587c-fbf5-4e03-bbfc-d94df647366f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}