{
  "annotation_id": "330f4469-e616-4db0-b6e7-a070a939ff6a",
  "date_created": "2026-03-02T18:00:24.521000Z",
  "date_modified": "2026-03-02T18:00:24.521000Z",
  "file_hash": "af5fd42b34db59652e485077dac8bb44109178afabdddc5d211e02a633100fc3",
  "private": false,
  "record": {
    "abstract": "We apply effective field theory and renormalization group techniques to the\nproblem of Cooper pair formation in neutron stars. Simple analytical\nexpressions for the $^1 S_0$ condensate are derived which are free of nuclear\npotential model dependencies. The condensate is evaluated using phase shift\ndata from neutron-neutron scattering.",
    "arxiv_id": "nucl-th/9811017",
    "authors": [
      "James Hormuzdiar",
      "Stephen Hsu"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "title": "Effective Field Theory of Neutron Star Superfluidity",
    "url": "https://arxiv.org/abs/nucl-th/9811017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8ca5e170-111a-459d-844e-dec3d394b59e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}