{
  "annotation_id": "9f117b16-cee4-4b4a-a82d-90c8ef8d9ea8",
  "date_created": "2026-03-02T18:00:11.264000Z",
  "date_modified": "2026-03-02T18:00:11.264000Z",
  "file_hash": "7802b111c71e603c1e46b47b9434da671b2c617862a591f31f40df796ef5dbf0",
  "private": false,
  "record": {
    "abstract": "The astrophysical $S$-factor for the reaction $^7$Be(p,$\\gamma$)$^8$B up to\nan energy of 2~MeV (c.m.) and the capture cross section of\n$^7$Li(n,$\\gamma$)$^8$Li up to 1~MeV (c.m.) are calculated using the Direct\nCapture model (DC). Both calculations are in good agreement with experimental\ndata.",
    "arxiv_id": "nucl-th/9301018",
    "authors": [
      "H. Krauss",
      "K. Gr\"un",
      "T. Rauscher",
      "H. Oberhummer"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1002/andp.19935050304",
    "journal_ref": "Ann. Phys. 505 (1993) 258-266; Annalen der Physik 2 (1993) 258-266",
    "title": "The Astrophysical S-Factor of the Reaction $^7$be(p,$\\gamma$)$^8$B in   the Direct Capture Model",
    "url": "https://arxiv.org/abs/nucl-th/9301018"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3c1ba0c4-0d0f-49eb-b7b8-44f99fec0c77",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}