{
  "annotation_id": "9758eb01-26df-4e48-af30-e4f72c794e34",
  "date_created": "2026-03-02T18:00:08.638000Z",
  "date_modified": "2026-03-02T18:00:08.638000Z",
  "file_hash": "53691c5bab2bf7312d2e237f39d9dfe172525d542ead29dd34fd5496e3d189f1",
  "private": false,
  "record": {
    "abstract": "The relation between energy and density (known as the nuclear equation of\nstate) plays a major role in a variety of nuclear and astrophysical systems.\nSpin and isospin asymmetries can have a dramatic impact on the equation of\nstate and possibly alter its stability conditions. An example is the possible\nmanifestation of ferromagnetic instabilities, which would indicate the\nexistence, at a certain density, of a spin-polarized state with lower energy\nthan the unpolarized one. This issue is being discussed extensively in the\nliterature and the conclusions are presently very model dependent. We will\nreport and discuss our recent progress in the study of spin-polarized neutron\nmatter. The approach we take is microscopic and relativistic. The calculated\nneutron matter properties are derived from realistic nucleon-nucleon\ninteractions. This makes it possible to understand the nature of the EOS\nproperties in terms of specific features of the nuclear force model.",
    "arxiv_id": "nucl-th/0607029",
    "authors": [
      "F. Sammarruca",
      "P. G. Krastev"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.75.034315",
    "journal_ref": "Phys.Rev.C75:034315,2007",
    "title": "Spin polarized neutron matter within the Dirac-Brueckner-Hartree-Fock   approach",
    "url": "https://arxiv.org/abs/nucl-th/0607029"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "4766cdaa-8933-4511-a657-c68c2af18f22",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}