{
  "annotation_id": "a958f1b2-d800-4194-a136-69b3288b5bb8",
  "date_created": "2026-03-02T18:00:04.338000Z",
  "date_modified": "2026-03-02T18:00:04.338000Z",
  "file_hash": "5e00772298f23da42b8f656c47d0d25b33bd4a9de1910e1841536d024b46771b",
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  "record": {
    "abstract": "The roles of isospin asymmetry in nuclei and neutron stars are investigated\nusing a range of potential and field-theoretical models of nucleonic matter.\nThe parameters of these models are fixed by fitting the properties of\nhomogeneous bulk matter and closed-shell nuclei. We discuss and unravel the\ncauses of correlations among the neutron skin thickness in heavy nuclei, the\npressure of beta-equilibrated matter at a density of 0.1 fm$^{-3}$, and the\nradii of moderate mass neutron stars. The influence of symmetry energy on\nobservables in heavy-ion collisions is summarized.",
    "arxiv_id": "nucl-th/0505062",
    "authors": [
      "Andrew W. Steiner",
      "Madappa Prakash",
      "James M. Lattimer",
      "Paul J. Ellis"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1556/APH.25.2006.2-4.8",
    "journal_ref": "Acta Phys.Hung. A25 (2006) 203-210",
    "title": "Isospin Asymmetry in Nuclei, Neutron Stars, and Heavy-Ion Collisions",
    "url": "https://arxiv.org/abs/nucl-th/0505062"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c0a8f059-8b8c-4396-ac75-e369c16edd36",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}