{
  "id": "1009.0976",
  "version": "v2",
  "published": "2010-09-06T07:14:56.000Z",
  "updated": "2013-02-21T05:30:55.000Z",
  "title": "Asymmetric Neutrino Emission from Magnetized Proto-Neutron Star Matter including Hyperons in Relativistic Mean Field Theory",
  "authors": [
    "Tomoyuki Maruyama",
    "Toshitaka Kajino",
    "Nobutoshi Yasutake",
    "Myung-Ki Cheoun",
    "Chung-Yeol Ryu"
  ],
  "comment": "9 pages, 3 figure",
  "journal": "Phys.Rev.D83:081303,2011",
  "doi": "10.1103/PhysRevD.83.081303",
  "categories": [
    "nucl-th",
    "astro-ph.SR"
  ],
  "abstract": "We calculate asymmetric neutrino absorption and scattering cross sections on hot and dense magnetized neutron-star matter including hyperons in fully relativistic mean field theory. The absorption/scattering cross sections are suppressed/enhanced incoherently in the direction of the magnetic fielld, B. The asymmetry is 2-4% at the matter density \\rho_0 < \\rho_B < 3\\rho_0 and temperature T < 40 MeV for B=2 X 10^{17} G. This asymmetry is comparable to the effects owing to parity violation or asymmetric magnetic field topology proposed for the origin of pulsar kicks.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2013-02-21T05:30:55.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "24.10.Jv",
      "26.60.-c",
      "25.30.Pt"
    ],
    "keywords": [
      "relativistic mean field theory",
      "magnetized proto-neutron star matter",
      "asymmetric neutrino emission"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Physical Review D",
      "year": 2011,
      "month": "Apr",
      "volume": 83,
      "number": 8,
      "pages": "081303"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 9,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 867231,
      "adsabs": "2011PhRvD..83h1303M"
    }
  }
}