{
  "annotation_id": "79a0a030-8481-470d-81af-738cdae1cc04",
  "date_created": "2026-03-02T18:00:08.578000Z",
  "date_modified": "2026-03-02T18:00:08.578000Z",
  "file_hash": "f51a59a58674db2eacecf2985679f1bafb98a94dc16a0f880b4b2e434de852a2",
  "private": false,
  "record": {
    "abstract": "We study the equation of state (EOS) for dense matter in the core of the\ncompact star with hyperons and calculate the star structure in an effective\nmodel in the mean field approach. With varying incompressibility and effective\nnucleon mass, we analyse the resulting EOS with hyperons in beta equilibrium\nand its underlying effect on the gross properties of the compact star\nsequences. The results obtained in our analysis are compared with predictions\nof other theoretical models and observations. The maximum mass of the compact\nstar lies in the range $1.21-1.96 ~M_{\\odot}$ for the different EOS obtained,\nin the model.",
    "arxiv_id": "nucl-th/0608013",
    "authors": [
      "T. K. Jha",
      "P. K. Raina",
      "P. K. Panda",
      "S. K. Patra"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.74.055803 10.1103/PhysRevC.75.029903",
    "journal_ref": "Phys.Rev.C74:055803,2006; Erratum-ibid.C75:029903,2007",
    "title": "Neutron star matter in an effective model",
    "url": "https://arxiv.org/abs/nucl-th/0608013"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6df11eef-9682-46f3-94c7-bd87643132eb",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}