{
  "annotation_id": "6fca1a7d-af91-4298-ad48-450e4126159b",
  "date_created": "2026-03-02T18:00:01.242000Z",
  "date_modified": "2026-03-02T18:00:01.242000Z",
  "file_hash": "e938a405e59473063e99eb0761dfe5910cdf19754ba47c7da261e46761959269",
  "private": false,
  "record": {
    "abstract": "The Trojan-Horse method is an indirect approach to determine the energy\ndependence of S factors of astrophysically relevant two-body reactions. This is\naccomplished by studying closely related three-body reactions under quasi-free\nscattering conditions. The basic theory of the Trojan-Horse method is developed\nstarting from a post-form distorted wave Born approximation of the T-matrix\nelement. In the surface approximation the cross section of the three-body\nreaction can be related to the S-matrix elements of the two-body reaction. The\nessential feature of the Trojan-Horse method is the effective suppression of\nthe Coulomb barrier at low energies for the astrophysical reaction leading to\nfinite cross sections at the threshold of the two-body reaction. In a modified\nplane wave approximation the relation between the two-body and three-body cross\nsections becomes very transparent. Applications of the Trojan Horse Method are\ndiscussed. It is of special interest that electron screening corrections are\nnegligible due to the high projectile energy.",
    "arxiv_id": "nucl-th/0401054",
    "authors": [
      "Gerhard Baur",
      "Stefan Typel"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "nucl-ex"
    ],
    "doi": "10.1143/PTPS.154.333",
    "journal_ref": "Prog.Theor.Phys.Suppl. 154 (2004) 333-340",
    "title": "Theory of the Trojan-Horse Method",
    "url": "https://arxiv.org/abs/nucl-th/0401054"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f3772220-0b29-433c-9859-b4e3daec4ab8",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}