{
  "annotation_id": "71fd4ef1-5697-4dcc-86eb-7f291126ea82",
  "date_created": "2026-03-02T18:00:08.637000Z",
  "date_modified": "2026-03-02T18:00:08.637000Z",
  "file_hash": "eff49d1a57ea103f7dca89edf6dfde041fc37d3604d6030cb2141bb74c2c0d47",
  "private": false,
  "record": {
    "abstract": "This chapter provides a review of microscopic theories of pairing in nuclear\nsystems and neutron stars. Special attention is given to the mean-field BCS\ntheory and its extensions to include effects of polarization of the medium and\nretardation of the interactions. Superfluidity in nuclear systems that exhibit\nisospin asymmetry is studied. We further address the crossover from the\nweak-coupling BCS description to the strong-coupling BEC limit in dilute\nnuclear systems. Finally, within the observational context of rotational\nanomalies of pulsars, we discuss models of the vortex state in superfluid\nneutron stars and of the mutual friction between superfluid and normal\ncomponents, along with the possibility of type-I superconductivity of the\nproton subsystem.",
    "arxiv_id": "nucl-th/0607028",
    "authors": [
      "Armen Sedrakian",
      "John W. Clark"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "cond-mat.supr-con"
    ],
    "doi": "10.1142/9789812773043_0006",
    "title": "Nuclear Superconductivity in Compact Stars: BCS Theory and Beyond",
    "url": "https://arxiv.org/abs/nucl-th/0607028"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a344f74d-d474-433c-b59a-39c368a90f9a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}