{
  "annotation_id": "1975d4e2-2988-4662-a5cf-691597549998",
  "date_created": "2026-03-02T18:00:22.404000Z",
  "date_modified": "2026-03-02T18:00:22.404000Z",
  "file_hash": "a9e481a81a6c7127a36abca2dfe4d5aa21ac1bfdaa7e25c72fa2a39c106d7480",
  "private": false,
  "record": {
    "abstract": "We present results obtained for nuclei, nuclear and neutron star matter, and\nneutron star structure obtained with the recent Argonne v18 two- nucleon and\nUrbana IX three-nucleon interactions including relativistic boost corrections.\nThese interactions predict that matter will undergo a transition to a spin\nlayered phase with neutral pion condensation. We also consider the possibility\nof a transition to quark matter.",
    "arxiv_id": "nucl-th/9802048",
    "authors": [
      "V. R. Pandharipande",
      "A. Akmal",
      "D. G. Ravenhall"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Many-body theory of nuclear and neutron star matter",
    "url": "https://arxiv.org/abs/nucl-th/9802048"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "eb003229-e153-4888-bfb3-997304dc9353",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}