{
  "annotation_id": "7c7e9ef0-85b3-4415-8f75-e434cda2816e",
  "date_created": "2026-03-02T18:00:42.867000Z",
  "date_modified": "2026-03-02T18:00:42.867000Z",
  "file_hash": "bfe6c09c3a6431b513d2e29727b0accdd5f039af2af1199da3f8db669f21f4d0",
  "private": false,
  "record": {
    "abstract": "We briefly examine the properties of dense plasmas characteristic of the\natmospheres of neutron stars and of the interior of massive white dwarfs. These\nastrophysical bodies are natural laboratories to study respectively the problem\nof pressure ionization of hydrogen in a strong magnetic field and the\ncrystallization of the quantum one-component-plasma at finite temperature.",
    "arxiv_id": "physics/0211089",
    "authors": [
      "G. Chabrier",
      "F. Douchin",
      "A. Y. Potekhin"
    ],
    "categories": [
      "physics.plasm-ph",
      "astro-ph"
    ],
    "doi": "10.1088/0953-8984/14/40/307",
    "journal_ref": "J.Phys.Condens.Matter 14 (2002) 9133",
    "title": "Dense astrophysical plasmas",
    "url": "https://arxiv.org/abs/physics/0211089"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "cffc7fae-2aa5-43f9-80b0-bd7a0b24a36a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}