{
  "annotation_id": "1278b4a9-aa42-4c90-9cea-491b0630e2e4",
  "date_created": "2026-03-02T18:00:08.427000Z",
  "date_modified": "2026-03-02T18:00:08.427000Z",
  "file_hash": "af69f176435e5bf7a1cbf5c517786e7fb9d695c9113ac152d5b8bc8443b5ca39",
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  "record": {
    "abstract": "Two of the key issues in understanding the neutron-to-proton ratio in a\ncore-collapse supernova are discussed. One of these is the behavior of the\nneutrino-nucleon cross sections as supernova energies. The other issue is the\nmany-body properties of the neutrino gas near the core when both one- and\ntwo-body interaction terms are included.",
    "arxiv_id": "nucl-th/0608047",
    "authors": [
      "A. B. Balantekin"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1088/1742-6596/49/1/022",
    "title": "Neutrinos, Weak Interactions, and r-process Nucleosynthesis",
    "url": "https://arxiv.org/abs/nucl-th/0608047"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "312b5a63-2b83-45e9-b960-28e98b018bb6",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}