{
  "annotation_id": "68160f5e-8b53-4ab7-aa2d-9cdbd63f2ab1",
  "date_created": "2026-03-02T18:00:25.356000Z",
  "date_modified": "2026-03-02T18:00:25.356000Z",
  "file_hash": "be648a8f3ec2cb349cf17a998d0386ec5d5016fbff398a5f69e0a270c4528453",
  "private": false,
  "record": {
    "abstract": "We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs\nby baryons in neutron stars employing a transport model in which neutrinos\ncouple to baryons with spectral width. The coherence effects, which are\nincluded by computing the self energies with fully dressed propagators, lead to\nthe Landau-Pomeranchuk-Migdal suppression of the neutrino emission rates in the\nsoft neutrino and high temperature limit. A microscopic evaluation of the\nbremsstrahlung rate by neutrons is carried out using the Brueckner theory of\nnuclear matter at finite temperatures.",
    "arxiv_id": "nucl-th/9905039",
    "authors": [
      "Armen Sedrakian",
      "Alex Dieperink"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1016/S0370-2693(99)00989-2",
    "journal_ref": "Phys.Lett. B463 (1999) 145-152",
    "title": "Coherence Effects and Neutrino Pair Bremsstrahlung in Neutron Stars",
    "url": "https://arxiv.org/abs/nucl-th/9905039"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3a9c0696-eb82-4b68-8abb-30ba98bfc8c5",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}