{
  "annotation_id": "92886cb6-bc02-4d30-8823-f70e06409378",
  "date_created": "2026-03-02T18:00:08.646000Z",
  "date_modified": "2026-03-02T18:00:08.646000Z",
  "file_hash": "932350b7434e46f5435cf473de5e2e3ba9f90b69c399fe58c1df5719d965d79b",
  "private": false,
  "record": {
    "abstract": "The nucleus of 208Pb -- a system that is 18 order of magnitudes smaller and\n55 orders of magnitude lighter than a neutron star -- may be used as a\nminiature surrogate to establish important correlations between its neutron\nskin and several neutron-star properties. Indeed, a nearly model-independent\ncorrelation develops between the neutron skin of 208Pb and the liquid-to-solid\ntransition density in a neutron star. Further, we illustrate how a measurement\nof the neutron skin in 208Pb may be used to place important constraints on the\ncooling mechanism operating in neutron stars and may help elucidate the\nexistence of quarks stars.",
    "arxiv_id": "nucl-th/0607039",
    "authors": [
      "J. Piekarewicz"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "nucl-ex"
    ],
    "title": "Neutron Rich Nuclei in Heaven and Earth: Proceedings of the   International Conference on Current Problems in Nuclear Physics and Atomic   Energy",
    "url": "https://arxiv.org/abs/nucl-th/0607039"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "5010808c-084b-4ef2-86eb-74c9a1c3ed9a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}