{
  "id": "0912.4311",
  "version": "v3",
  "published": "2009-12-22T01:28:24.000Z",
  "updated": "2010-03-25T04:32:53.000Z",
  "title": "Classical gauge field as a dark matter",
  "authors": [
    "V. Dzhunushaliev",
    "K. Myrzakulov",
    "R. Myrzakulov"
  ],
  "comment": "changes in the text, Fig.4 is repainted",
  "categories": [
    "astro-ph.CO"
  ],
  "abstract": "The model of dark matter is presented where the dark matter is a \\emph{classical} gauge field. A spherical symmetric solution of Yang-Mills equation is obtained. The asymptotic behavior of the gauge fields and matter density is investigated. It is shown that the distribution of the matter density allows us interpret it as the dark matter. The fitting of a typical rotational curve with the rotational curve created by the spherical solution of SU(3) Yang-Mills equation is made.",
  "revisions": [
    {
      "version": "v3",
      "updated": "2010-03-25T04:32:53.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "11.27.+d",
      "95.35.+d"
    ],
    "keywords": [
      "dark matter",
      "classical gauge field",
      "yang-mills equation",
      "matter density",
      "spherical symmetric solution"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 840952,
      "adsabs": "2009arXiv0912.4311D"
    }
  }
}