{
  "annotation_id": "928a9075-f10a-4e65-920a-1c0d928a5414",
  "date_created": "2026-03-02T18:00:29.340000Z",
  "date_modified": "2026-03-02T18:00:29.340000Z",
  "file_hash": "e39449676637c6c6ec2fc22fc78f5d348bc2db865c7e75062ec783efd90dab8c",
  "private": false,
  "record": {
    "abstract": "Nonextensive and quantum uncertainty effects (related to the quasiparticles\ncomposing the stellar core) have strong influence on the nuclear rates and, of\ncourse, affect solar neutrino fluxes. Both effects do coexist and are due to\nthe frequent collisions among the ions. The weakly nonextensive nature of the\nsolar core is confirmed. The range of predictions for the neutrino fluxes is\nenlarged and the solar neutrino problem becomes less dramatic.",
    "arxiv_id": "nucl-th/9912064",
    "authors": [
      "A. Lavagno",
      "P. Quarati"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "cond-mat.stat-mech",
      "hep-ph"
    ],
    "doi": "10.1016/S0920-5632(00)00669-1",
    "journal_ref": "Nucl.Phys.Proc.Suppl. 87 (2000) 209-211",
    "title": "Nonextensive statistics in stellar plasma and solar neutrinos",
    "url": "https://arxiv.org/abs/nucl-th/9912064"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "daf650d2-e6aa-42cd-a147-27956f95fd99",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}