{
  "id": "1110.2293",
  "version": "v2",
  "published": "2011-10-11T07:41:17.000Z",
  "updated": "2011-11-28T14:35:48.000Z",
  "title": "Neutrinos as Hot or Warm Dark Matter",
  "authors": [
    "Y. F. Li",
    "Zhi-zhong Xing"
  ],
  "comment": "10 pages, 5 figures, references updated, published in Acta Phys. Polon. B 42, 2193 (2011)",
  "journal": "Acta Phys. Polon. B 42, 2193 (2011)",
  "categories": [
    "hep-ph",
    "astro-ph.CO"
  ],
  "abstract": "Both active and sterile sub-eV neutrinos can serve for hot dark matter (DM). On the other hand, keV sterile neutrinos could be a good candidate for warm DM. The beta-decaying (e.g., H-3 and Ru-106) and EC-decaying (e.g., Ho-163) nuclei are considered as the most promising targets to capture those extremely low energy neutrinos and antineutrinos, respectively. We calculate the capture rates of relic electron neutrinos and antineutrinos against the corresponding beta-decay or EC-decay backgrounds in different flavor mixing schemes. We stress that such direct laboratory measurements of hot or warm DM might not be hopeless in the long term.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2011-11-28T14:35:48.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "14.60.Pq",
      "13.15.+g",
      "14.60.St",
      "95.35.+d"
    ],
    "keywords": [
      "warm dark matter",
      "warm dm",
      "relic electron neutrinos",
      "extremely low energy neutrinos",
      "hot dark matter"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.5506/APhysPolB.42.2193"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 939514,
      "adsabs": "2011arXiv1110.2293L"
    }
  }
}