{
  "annotation_id": "95d207d8-ef5f-4b1f-9592-8e47d5cbfead",
  "date_created": "2026-03-02T18:00:11.328000Z",
  "date_modified": "2026-03-02T18:00:11.328000Z",
  "file_hash": "9a79c7d4d5384a05383fe1754591429a78f016522b8834afab20bad4415a4e8a",
  "private": false,
  "record": {
    "abstract": "We present some results and remarks based on a combinatorial approach of the\nevaluation of the nuclear level density. First, we show that it is possible to\nextract some reliable information from the output of the program whose rough\ndata present a strong statistical fluctuation from bin to bin. This includes\nsmoothing and evaluation of the desired quantities. After some comments about\nthe spin and parity distributions, we consider the question of the\nnon-equipartition of parities, mainly, at low energies. Finally, we present a\nsimple model to include and test this effect in the computation of\nthermonuclear reaction rates.",
    "arxiv_id": "nucl-th/9309025",
    "authors": [
      "Bernard PICHON CNRS"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "title": "Combinatorial Study of Nuclear Level Density for Astrophysical   Applications",
    "url": "https://arxiv.org/abs/nucl-th/9309025"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "051720c8-ef21-4f5e-9cc6-f310639b66c6",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}