{
  "annotation_id": "acc7455b-8020-49f0-be6f-d1c1ba04c299",
  "date_created": "2026-03-02T18:00:07.828000Z",
  "date_modified": "2026-03-02T18:00:07.828000Z",
  "file_hash": "c3a5bde34e6eb2aec082bac6dbb2205d84145ffbb60e0b49b80f7a19cfb69035",
  "private": false,
  "record": {
    "abstract": "The Trojan Horse (TH) method is a powerful indirect technique that provides\ninformation to determine astrophysical factors for rearrangement processes at\nastrophysically relevant energies. A short coming for understanding the\nreliability of the technique has been determining the importance of nuclear and\nCoulomb effects on the energy dependence of the yield. Using a simple model, we\ndemonstrate that off-energy-shell and Coulomb effects in the entry channel and\nthe final state nuclear interactions do not change the energy dependence of the\nastrophysical factor extracted from the TH reaction. Some examples are\npresented.",
    "arxiv_id": "nucl-th/0602001",
    "authors": [
      "A. M. Mukhamedzhanov",
      "C. Spitaleri",
      "R. E. Tribble"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "The Trojan Horse Method: an Indirect Technique in Nuclear Astrophysics",
    "url": "https://arxiv.org/abs/nucl-th/0602001"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6251d1ef-f874-45e0-9912-de0a18c5c427",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}