{
  "annotation_id": "50c9f27e-4df5-45c1-bb10-d3a58ff2987d",
  "date_created": "2026-03-02T18:00:18.401000Z",
  "date_modified": "2026-03-02T18:00:18.401000Z",
  "file_hash": "864c6adb44fa5d72146baf4cf14d54ea6a606b27917b0eb4a5561e3c01c759dd",
  "private": false,
  "record": {
    "abstract": "The present status of the nuclear reaction rates determining the solar\nneutrino flux is discussed. This includes the reaction rates for the two\nbranching ratios of the three pp-chains involving the reactions 3He(3He,2p)4He\nand 3He(4He,gamma)7Be for the first branching, and 7Be(e-,nu_e)7Li and\n7Be(p,gamma)7B for the second branching. Mainly we will concentrate on the\nbasic nuclear reaction p + p -\u003e D + e+ + nu_e of the pp-chains. We use a\nrelativistic field theory model of the deuteron to calculate the low-energy\ncross section for this reaction. The theoretical prediction of the cross\nsection obtained is about 2.9 times largerthan given in the conventional\npotential approach. The consequences of this new reaction rate for the solar\nneutrino problem will be presented and discussed.",
    "arxiv_id": "nucl-th/9705046",
    "authors": [
      "H. Oberhummer",
      "A. N. Ivanov",
      "N. I. Troitskaya",
      "M. Faber"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1023/A:1001783223339",
    "journal_ref": "Astrophys.SpaceSci.258:133-144,1998",
    "title": "Nuclear aspects of the solar neutrino problem",
    "url": "https://arxiv.org/abs/nucl-th/9705046"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a54d8971-c574-49fe-bc4f-4d5f11118ea5",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}