{
  "annotation_id": "e9f12e89-81b7-4b7a-b47e-528922a166e4",
  "date_created": "2026-03-02T18:00:22.144000Z",
  "date_modified": "2026-03-02T18:00:22.144000Z",
  "file_hash": "a0e5827b4ab296089c567e370f33079b59f328e62f513d6dc45c3602473f96d2",
  "private": false,
  "record": {
    "abstract": "We explore approximations to the effective $S$ factor for the\n$^7Be(p,\\gamma)^8B$ reaction using different approximation for the integral\nover the Gamov peak. In the temperature range of interest for solar neutrino\nproduction, $S_{eff}(E)$ may be determined to within 0.5% from S(20) with no\ndirect information on the derivatives of S(E).",
    "arxiv_id": "nucl-th/9807007",
    "authors": [
      "B. K. Jennings",
      "S. Karataglidis"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.58.3002",
    "journal_ref": "Phys.Rev.C58:3002-3003,1998",
    "title": "S_eff(E) and the 7Be(p,gamma)8B reaction",
    "url": "https://arxiv.org/abs/nucl-th/9807007"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "1f5e18dd-5564-4e1e-af27-dc4a0edd6914",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}