{
  "annotation_id": "5401236d-7c6e-489f-af35-f2657944c895",
  "date_created": "2026-03-02T18:00:03.933000Z",
  "date_modified": "2026-03-02T18:00:03.933000Z",
  "file_hash": "5cd4071c4f7980c650955a1ba44896c163ed78b5ae71ad9b6b66d4f7b3d6f90c",
  "private": false,
  "record": {
    "abstract": "REACLIB is one of the most comprehensive and popular astrophysical reaction\nrate libraries. However, its experimentally obtained rates for light isotopes\nstill rely mainly on the Caughlan \u0026 Fowler (1988) compilation and have never\nbeen updated despite the progress in many relevant nuclear astrophysics\nexperiments. Moreover, due to fitting errors REACLIB is not reliable at\ntemperatures lower than 10^{7}K. In this work we establish the formalism for\nupdating the obsolete Caughlan-Fowler experimental rates of REACLIB. Then we\nuse the NACRE compilation and results from the LUNA experiments to update some\nimportant charged-particle induced rates of REACLIB focusing on the\nproton-proton chain. The updated rates (available also in digital form) can now\nbe used in the low temperature regime (below 10^{7}K) which was forbidden to\nthe old version of REACLIB.",
    "arxiv_id": "nucl-th/0502013",
    "authors": [
      "Theodore E. Liolios"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "title": "Updating the nuclear reaction rate library REACLIB. (I. Experimental   reaction rates of the proton-proton chain)",
    "url": "https://arxiv.org/abs/nucl-th/0502013"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "4eebc645-0664-407c-a661-121b1d368a95",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}