{
  "id": "1801.09554",
  "version": "v1",
  "published": "2018-01-25T20:46:08.000Z",
  "updated": "2018-01-25T20:46:08.000Z",
  "title": "Neutrinos, supernovae, and the origin of the heavy elements",
  "authors": [
    "Yong-Zhong Qian"
  ],
  "comment": "6 pages, 2 figures",
  "journal": "Sci. China-Phys. Mech. Astron. 61 (2018) 049501",
  "doi": "10.1007/s11433-017-9142-2",
  "categories": [
    "astro-ph.HE",
    "astro-ph.SR",
    "hep-ph",
    "nucl-th"
  ],
  "abstract": "Stars of ~8-100 solar masses end their lives as core-collapse supernovae (SNe). In the process they emit a powerful burst of neutrinos, produce a variety of elements, and leave behind either a neutron star or a black hole. The wide mass range for SN progenitors results in diverse neutrino signals, explosion energies, and nucleosynthesis products. A major mechanism to produce nuclei heavier than iron is rapid neutron capture, or the r process. This process may be connected to SNe in several ways. A brief review is presented on current understanding of neutrino emission, explosion, and nucleosynthesis of SNe.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-01-25T20:46:08.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "heavy elements",
      "produce nuclei heavier",
      "solar masses end",
      "sn progenitors results",
      "diverse neutrino signals"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "Springer"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}