{
  "annotation_id": "7c2c22ad-c3bc-4575-bc6b-1d4b3cbc1723",
  "date_created": "2026-03-02T18:00:14.862000Z",
  "date_modified": "2026-03-02T18:00:14.862000Z",
  "file_hash": "62f2b026e63f445f7a85650deb60bed5194ce7beb80c7e2948f1ebee51e86474",
  "private": false,
  "record": {
    "abstract": "We have studied the properties of A=54 and A=64 isobars at temperatures T\n\\leq 2 MeV via Monte Carlo shell model calculations with two different residual\ninteractions. In accord with empirical indications, we find that the symmetry\nenergy coefficient, b_{sym}, is independent of temperature to within 0.6 MeV\nfor T \\leq 1 MeV. This is in contrast to a recent suggestion of a 2.5 MeV\nincrease of b_{sym} for this temperature, which would have significantly\naltered the supernova explosion scenario.",
    "arxiv_id": "nucl-th/9408026",
    "authors": [
      "D. J. Dean",
      "S. E. Koonin",
      "K. Langanke",
      "P. B. Radha"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0370-2693(95)00858-I",
    "journal_ref": "Phys.Lett. B356 (1995) 429-433",
    "title": "Temperature dependence of the nuclear symmetry energy",
    "url": "https://arxiv.org/abs/nucl-th/9408026"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7dd65f16-9c50-481c-a425-56d0225b8a8c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}