{
  "id": "nucl-th/0201026",
  "version": "v2",
  "published": "2002-01-11T14:09:58.000Z",
  "updated": "2002-01-14T10:31:43.000Z",
  "title": "Fragment Distribution in Coexistence Phase of Supernova Matter",
  "authors": [
    "Chikako Ishizuka",
    "Akira Ohnishi",
    "Kousuke Sumiyoshi"
  ],
  "comment": "5 pages, 3 figures, proceedings of Yukawa International Seminar 2001 (YKIS01), Physics of Unstable Nuclei, November 5-10, 2001, Kyoto, Japan. (v2: minor package change to adapt ptptex style file.)",
  "journal": "Prog.Theor.Phys.Suppl.146:373-377,2003",
  "doi": "10.1143/PTPS.146.373",
  "categories": [
    "nucl-th",
    "astro-ph"
  ],
  "abstract": "We propose a new nucleosynthesis process in which various nuclei are formed through the liquid-gas phase transition of supernova matter as a preprocess of the standard r-process, and study its possibility of realization qualitatively. In the relativistic mean field and statistical model calculations, we find that this process may take place and help the later r-process to proceed.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2002-01-14T10:31:43.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "supernova matter",
      "coexistence phase",
      "fragment distribution",
      "liquid-gas phase transition",
      "relativistic mean field"
    ],
    "tags": [
      "research tool",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 581671
    }
  }
}