{
  "annotation_id": "ebde89d4-f56c-40c2-a713-9a7f6b290317",
  "date_created": "2026-03-02T18:00:18.208000Z",
  "date_modified": "2026-03-02T18:00:18.208000Z",
  "file_hash": "0609256cda7435cd6c963205a8c7cb8300fe8ca6c08175972a49fade5f90fba4",
  "private": false,
  "record": {
    "abstract": "The nuclear reaction e+p+d -----\u003e He3 + e is considered at thermonuclear\nenergies. The motion of the electron is treated within the adiabatic\napproximation and the pd scattering state is constructed in the form of an\nantisymmetrized product of the bound state wave function of the deuteron and of\nthe wave function of the pd relative motion. The latter is calculated using an\neffective pd potential constructed via the Marchenko inverse scattering method.\nThe bound state wave function of He3 is obtained using Faddeev--type\nintegrodifferential equations. The reaction rate thus obtained for the solar\ninterior conditions is approximately 10^{-4} of the corresponding rate for the\nradiative capture pd ----\u003e He3 + gamma .",
    "arxiv_id": "nucl-th/9607027",
    "authors": [
      "S. A. Rakityansky",
      "S. A. Sofianos",
      "L. L. Howell",
      "M. Braun",
      "V. B. Belyaev"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "plasm-ph"
    ],
    "doi": "10.1016/S0375-9474(96)00413-7",
    "journal_ref": "Nucl.Phys. A613 (1997) 132-146",
    "title": "Nonradiative proton--deuteron fusion in stellar plasma",
    "url": "https://arxiv.org/abs/nucl-th/9607027"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "1a802686-218e-4eec-910e-5f4e4c5e6e56",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}