{
  "annotation_id": "9347538b-608b-4f4d-8454-edf4ff8b350c",
  "date_created": "2026-03-02T18:00:14.934000Z",
  "date_modified": "2026-03-02T18:00:14.934000Z",
  "file_hash": "e3eb2a4dcb694775666611ec106d0c1bb52c671b0381c14f63f5a95cf79b25b6",
  "private": false,
  "record": {
    "abstract": "The relationship between the Coulomb displacement energy for the A=8, J=2+,\nT=1 state and the low-energy astrophysical S factor for the Be7(p,gamma)B8\nreaction is discussed. The displacement energy is interpreted in a\nparticle-hole model. The dependence of the particle displacement energy on the\npotential well geometry is investigated and is used to relate the particle\ndisplacement energy to the rms radius and the asymptotic normalization of the\nvalence proton wave function in B8. The asymptotic normalization is used to\ncalculate the astrophysical S factor for the Be7(p,gamma)B8 reaction. The\nrelationship to the Li7(n,gamma) reaction, the B8 quadrupole moment, radial\ndensity, and break-up momentum distribution are also discussed.",
    "arxiv_id": "nucl-th/9506004",
    "authors": [
      "B. A. Brown",
      "A. Csoto",
      "R. Sherr"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1016/0375-9474(95)00417-3",
    "journal_ref": "Nucl.Phys.A597:66-84,1996",
    "title": "Coulomb displacement energy and the low-energy astrophysical S factor   for the Be7(p,gamma)B8 reaction",
    "url": "https://arxiv.org/abs/nucl-th/9506004"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8dc971b9-3fba-4425-bca0-fafdb58ff0ca",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}