{
  "annotation_id": "11cb6241-13a9-48ec-8498-4ac9874c5ef8",
  "date_created": "2026-03-02T18:00:07.689000Z",
  "date_modified": "2026-03-02T18:00:07.689000Z",
  "file_hash": "f58e50d32fc27e794c6755dd2d3e0b154e4761913cb5b555fbf0f18eff0694a9",
  "private": false,
  "record": {
    "abstract": "A new shell model Hamiltonian for p-shell nuclei which properly takes into\naccount important roles of spin-isospin interactions is used to obtain cross\nsections of neutrino-^12C reactions induced by decay-at-rest (DAR) neutrinos as\nwell as supernona neutrinos. Branching ratios to various decay channels are\ncalculated by the Hauser-Feshbach theory. Neutrino-^4He reactions are also\ninvestigated by using recent shell model Hamiltonians. The reaction cross\nsections are found to be enhanced for both ^12C and ^4He compared with previous\ncalculations. As an interesting consequence of this, a possible enhancement of\nthe production yields of light elements, ^7Li and ^11B, during supernova\nexplosions is pointed out.",
    "arxiv_id": "nucl-th/0608056",
    "authors": [
      "Toshio Suzuki",
      "Satoshi Chiba",
      "Takashi Yoshida",
      "Toshitaka Kajino",
      "Takaharu Otsuka"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.74.034307",
    "journal_ref": "Phys.Rev.C74:034307,2006",
    "title": "Neutrino Nucleus Reactions based on New Shell Model Hamiltonians",
    "url": "https://arxiv.org/abs/nucl-th/0608056"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "326d8c3b-4af7-4bdc-b8fa-2c3c53052393",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}