{
  "annotation_id": "b7a17c08-e19d-4976-8018-152dd9f95bde",
  "date_created": "2026-03-02T18:00:18.806000Z",
  "date_modified": "2026-03-02T18:00:18.806000Z",
  "file_hash": "428db4a1ea385e7dbef6c7145e4fc691f5e4858a7d63d1403aa2ed639958dbe0",
  "private": false,
  "record": {
    "abstract": "We calculate the reaction cross-sections for the fusion of hydrogen and\ndeuterium in strong magnetic fields as are believed to exist in the atmospheres\nof neutron stars. We find that in the presence of a strong magnetic field ($B\n\\gsim 10^{12}$G), the reaction rates are many orders of magnitude higher than\nin the unmagnetized case. The fusion of both protons and deuterons are\nimportant over a neutron star\u0027s lifetime for ultrastrong magnetic fields ($B\n\\sim 10^{16}$G). The enhancement may have dramatic effects on thermonuclear\nrunaways and bursts on the surfaces of neutron stars.",
    "arxiv_id": "nucl-th/9608054",
    "authors": [
      "Jeremy S. Heyl",
      "Lars Hernquist"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.54.2751",
    "journal_ref": "Phys.Rev.C54:2751-2759,1996",
    "title": "Magnetically Catalyzed Fusion",
    "url": "https://arxiv.org/abs/nucl-th/9608054"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "93295f8f-704f-4640-b30e-8a45b8aef535",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}