{
  "annotation_id": "9ae8fdf6-609b-49ec-9775-9901fe6ff24f",
  "date_created": "2026-03-02T18:00:04.905000Z",
  "date_modified": "2026-03-02T18:00:04.905000Z",
  "file_hash": "bb1ce44ba7ed82c4c992c0d5804d39e540a8e0a78c84f9dfac8bf7b2068409e5",
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  "record": {
    "abstract": "Nuclear structure data are of crucial importance in order to address\nimportant astrophysical problems such as the origin of chemical elements, the\ninner working of our Sun, and the evolution of stars. We demonstrate this by\ninvestigating the ground state structure of $^8$B and $^7$Be nuclei within the\nSkyrme Hartree-Fock framework and by calculating the overlap integral of $^8$B\nand $^7$Be wave functions. The latter is used to calculate the astrophysical S\nfactor ($S_{17}$) for the solar fusion reaction $^{7}$Be($p, \\gamma)^{8}$B.",
    "arxiv_id": "nucl-th/0504062",
    "authors": [
      "Shashi K. Dhiman",
      "R. Shyam"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1088/0954-3899/31/10/026",
    "journal_ref": "J.Phys. G31 (2005) S1531-S1536",
    "title": "Structure of $^8$B and astrophysical $S_{17}$ factor",
    "url": "https://arxiv.org/abs/nucl-th/0504062"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c5c54e80-0f45-4a46-91cd-4d66c4994a3b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}