{
  "annotation_id": "cc880089-6db0-409f-a744-dc9dcdb859e4",
  "date_created": "2026-03-02T18:00:22.208000Z",
  "date_modified": "2026-03-02T18:00:22.208000Z",
  "file_hash": "0e5dd35e6411bca50f0a00b62ab7cdb54eb141d97e22738b21a0aecee031ccbd",
  "private": false,
  "record": {
    "abstract": "We discuss microscopic cluster model descriptions of two solar nuclear\nreactions, Be7(p,gamma)B8 and He3(He3,2p)He4. The low-energy reaction cross\nsection of Be7(p,gamma)B8, which determines the high-energy solar neutrino\nflux, is constrained by Be7 and B8 observables. Our results show that a small\nvalue of the zero-energy cross section is rather unlikely. In He3(He3,2p)He4 we\nstudy the effects of a possible virtual state on the cross section. Although,\nwe have found no indication for such a state so far, its existence cannot be\nruled out yet. We calculate the He3(He3,2p)He4 and H3(H3,2n)He4 cross sections\nin a continuum-discretized coupled channel approximation, and find a good\ngeneral agreement with the data.",
    "arxiv_id": "nucl-th/9712033",
    "authors": [
      "Attila Csoto"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "nucl-ex"
    ],
    "journal_ref": "Proceedings published by World Scientific, page 214 (1998)",
    "title": "Nuclear physics input for solar models",
    "url": "https://arxiv.org/abs/nucl-th/9712033"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a4ddeaeb-596b-4e6e-80aa-126ea9fee81a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}