{
  "annotation_id": "e3adb307-c443-4b09-a411-c81348d16c73",
  "date_created": "2026-03-02T18:00:15.419000Z",
  "date_modified": "2026-03-02T18:00:15.419000Z",
  "file_hash": "564b5e1d5eec9cdaab3026c77c1c7ea9cc2792e9655b079dc0c9f53f9c96ae68",
  "private": false,
  "record": {
    "abstract": "I show that the solar neutrino fluxes, predicted by standard nuclear and\nsolar physics, can get closer to the experimental observations if one takes the\nfreedom to introduce two free parameters into the model, as it is done in the\nMSW solution. I point out that the plasma electron capture of Be7 and the\nHe3(He3,2p)He4 nuclear reactions deserve further experimental and theoretical\nattention.",
    "arxiv_id": "nucl-th/9505034",
    "authors": [
      "Attila Csoto"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "title": "On the balance of the solar p-p chain",
    "url": "https://arxiv.org/abs/nucl-th/9505034"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a7133802-0fce-4609-a75b-a89191f4a562",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}