{
  "annotation_id": "83bc3030-a040-45a3-b444-c2fd65818e19",
  "date_created": "2026-03-02T18:00:22.202000Z",
  "date_modified": "2026-03-02T18:00:22.202000Z",
  "file_hash": "69bbec53bb3889735a0eb3faafe9197e81861f81b1a38e98bf5f86965405d668",
  "private": false,
  "record": {
    "abstract": "Several nuclear reactions involving the Be7 nucleus, not included into the\nstandard model of the pp-chain, are discussed. A qualitative analysis of their\npossible influence on the fate of the Be7 in solar plasma and of their role in\nthe interpretation of the solar neutrino experiments is given. As an example,\nthe reaction rate of the nonradiative production of B8 in the triple collision\np + e^- + Be7 ---\u003e B8 + e^- is estimated in the framework of the adiabatic\napproximation. For the solar interior conditions the triple collision reaction\nrate is approximately 10^{-4} of that for the binary process p + Be7 ---\u003e B8 +\ngamma .",
    "arxiv_id": "nucl-th/9712020",
    "authors": [
      "D. E. Monakhov",
      "V. B. Belyaev",
      "S. A. Sofianos",
      "S. A. Rakityansky",
      "W. Sandhas"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1016/S0375-9474(98)00174-2",
    "journal_ref": "Nucl.Phys. A635 (1998) 257-269",
    "title": "Triple collisions (e+p+Be7) in solar plasma",
    "url": "https://arxiv.org/abs/nucl-th/9712020"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0ef226ca-6c54-488a-876a-f9dd2a9b9d6a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}