{
  "id": "1602.04338",
  "version": "v1",
  "published": "2016-02-13T14:28:58.000Z",
  "updated": "2016-02-13T14:28:58.000Z",
  "title": "Capture cross sections of 15N(n, γ)16N at astrophysical energies",
  "authors": [
    "Guang-wei Fan",
    "Jun-bing Ma",
    "Zong-qiang Sheng",
    "Feng Tian",
    "Jun Wang",
    "Chao Zhang"
  ],
  "comment": "5 pages, 3 figures",
  "categories": [
    "nucl-th"
  ],
  "abstract": "We have reanalyzed reaction cross sections of 16N on 12C target. The nucleon density distribution of 16N, especially surface density distribution, was extracted using the modified Glauber model. On the basis of dilute surface densities, the discussion of 15N(n, {\\gamma})16N reaction was performed within the framework of the direct capture reaction mechanism. The calculations agreed quite well with the experimental data.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-02-13T14:28:58.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "capture cross sections",
      "astrophysical energies",
      "direct capture reaction mechanism",
      "nucleon density distribution",
      "reanalyzed reaction cross sections"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1421682
    }
  }
}