{
  "annotation_id": "60e3101f-76b4-4a38-a2fd-791e1d8cc366",
  "date_created": "2026-03-02T18:00:11.919000Z",
  "date_modified": "2026-03-02T18:00:11.919000Z",
  "file_hash": "a0887e839bc2318d29a81cd9750bdbce043e36aa44cc0a5238f4fff14429710d",
  "private": false,
  "record": {
    "abstract": "Because of the presence of a liquid-gas phase transition in nuclear matter,\ncompact-star matter can present a region of instability against the formation\nof clusters. We investigate this phase separation in a matter composed of\nneutrons, protons and electrons, within a Skyrme-Lyon mean-field approach.\nMatter instability and phase properties are characterized through the study of\nthe free-energy curvature. The effect of beta-equilibrium is also analyzed in\ndetail, and we show that the opacity to neutrinos has an influence on the\npresence of clusterized matter in finite-temperature proto-neutron stars.",
    "arxiv_id": "nucl-th/0612044",
    "authors": [
      "Camille Ducoin",
      "Philippe Chomaz",
      "Francesca Gulminelli"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1016/j.nuclphysa.2007.03.006",
    "journal_ref": "Nucl.Phys.A789:403-425,2007",
    "title": "Isospin-dependent clusterization of Neutron-Star Matter",
    "url": "https://arxiv.org/abs/nucl-th/0612044"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b7b00a7e-c48c-4276-8e9e-1e6ea0d6b5e9",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}