{
  "annotation_id": "ef424b8b-c1a6-4b15-91ec-52d58b68ef8f",
  "date_created": "2026-03-02T18:00:08.115000Z",
  "date_modified": "2026-03-02T18:00:08.115000Z",
  "file_hash": "84f942751094b15722e2d49998d24444c90ec7081d37835a712adf84c88341b1",
  "private": false,
  "record": {
    "abstract": "The thermodynamics properties of globally neutral dense stellar matter are\nanalyzed both in terms of mean field instabilities and structures beyond the\nmean field. The mean field response to finite wavelenght fluctuations is\ncalculated with the realistic Sly230a effective interaction. A Monte Carlo\nsimulation of a schematic lattice Hamiltonian shows the importance of\ncalculations beyond the mean field to calculate the phase diagram of stellar\nmatter. The analogies and differences respect to the thermodynamics of nuclear\nmatter and finite nuclei are stressed.",
    "arxiv_id": "nucl-th/0605042",
    "authors": [
      "F. Gulminelli",
      "P. Chomaz",
      "C. Ducoin",
      "P. Napolitani",
      "K. Hasnaoui"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1063/1.2710599",
    "journal_ref": "AIPConf.Proc.884:318-326,2007",
    "title": "From multifragmentation to supernovae and neutron stars",
    "url": "https://arxiv.org/abs/nucl-th/0605042"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c4cbd798-3b9a-4c93-a20b-c32ef985f6d0",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}