{
  "annotation_id": "af5a7764-769d-427a-9da5-409622f6a991",
  "date_created": "2026-03-02T18:00:10.880000Z",
  "date_modified": "2026-03-02T18:00:10.880000Z",
  "file_hash": "6e4a37fd622a865e25063c859978af3ea36e2bb7debabd34b55f7e76c7b58077",
  "private": false,
  "record": {
    "abstract": "During the collapse of massive stars, and the supernova type-II explosions,\nstellar matter reaches densities and temperatures which are similar to the ones\nobtained in intermediate-energy nucleus-nucleus collisions. The nuclear\nmultifragmentation reactions can be used for determination of properties of\nnuclear matter at subnuclear densities, in the region of the nuclear liquid-gas\nphase transition. It is demonstrated that the modified properties of hot nuclei\n(in particular, their symmetry energy) extracted from the multifragmentation\ndata can essentially influence nuclear composition of stellar matter. The\neffects on weak processes, and on the nucleosynthesis are also discussed.",
    "arxiv_id": "nucl-th/0612055",
    "authors": [
      "A. S. Botvina",
      "I. N. Mishustin",
      "W. Trautmann"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "title": "Properties of stellar matter in supernova explosions and nuclear   multifragmentation",
    "url": "https://arxiv.org/abs/nucl-th/0612055"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "86a1e3ee-a965-4c26-b891-ceb73f530491",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}