{
  "id": "1112.6328",
  "version": "v1",
  "published": "2011-12-29T15:28:50.000Z",
  "updated": "2011-12-29T15:28:50.000Z",
  "title": "Strange matter in core-collapse supernovae",
  "authors": [
    "I. Sagert",
    "T. Fischer",
    "M. Hempel",
    "G. Pagliara",
    "J. Schaffner-Bielich",
    "F. -K. Thielemann",
    "M. Liebendörfer"
  ],
  "comment": "8 pages, 3 figures, Invited talk at the \"Strangeness in Quark Matter\" conference, 18-24 September 2011, Polish Academy of Arts and Sciences, Cracow, Poland",
  "journal": "Acta Physica Polonica B vol. 43 (2012) page 741",
  "doi": "10.5506/APhysPolB.43.741",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We discuss the possible impact of strange quark matter on the evolution of core-collapse supernovae with emphasis on low critical densities for the quark-hadron phase transition. For such cases the hot proto-neutron star can collapse to a more compact hybrid star configuration hundreds of milliseconds after core-bounce. The collapse triggers the formation of a second shock wave. The latter leads to a successful supernova explosion and leaves an imprint on the neutrino signal. These dynamical features are discussed with respect to their compatibility with recent neutron star mass measurements which indicate a stiff high density nuclear matter equation of state.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-12-29T15:28:50.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "25.75.Nq",
      "21.65.Qr",
      "26.60.-c",
      "12.38.-t"
    ],
    "keywords": [
      "core-collapse supernovae",
      "strange matter",
      "stiff high density nuclear matter",
      "compact hybrid star configuration hundreds",
      "high density nuclear matter equation"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1083052,
      "adsabs": "2011arXiv1112.6328S"
    }
  }
}