{
  "annotation_id": "280e637b-c398-4d4b-bd56-b49dc13d50da",
  "date_created": "2026-03-02T18:00:01.186000Z",
  "date_modified": "2026-03-02T18:00:01.186000Z",
  "file_hash": "5708f01197e9912c70ff50acc5f7379f6f281806ae764bc0e0fc262cab5b7f28",
  "private": false,
  "record": {
    "abstract": "The Feshbach theory of the optical potential naturally leads to a microscopic\ndescription of scattering in terms of the many-body self-energy. We consider a\nrecent calculation of this quantity for 16O and study the possibility of\napplying it at astrophysical energies. The results obtained for the phase\nshifts and the 16O(p,\\gamma) capture suggest that such studies are feasible but\nthe calculations require some improvement geared to this specific task.",
    "arxiv_id": "nucl-th/0408017",
    "authors": [
      "C. Barbieri",
      "B. K. Jennings"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/j.nuclphysa.2005.05.071",
    "journal_ref": "Nucl.Phys. A758 (2005) 395-398",
    "title": "Study of the 16O(p,gamma) Reaction at Astrophysical Energies",
    "url": "https://arxiv.org/abs/nucl-th/0408017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "da38e93e-17bb-4692-bcde-552b20d0cf5a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}