{
  "id": "1909.08861",
  "version": "v1",
  "published": "2019-09-19T08:43:06.000Z",
  "updated": "2019-09-19T08:43:06.000Z",
  "title": "Dark Matter Mass and Anisotropy in Directional Detector",
  "authors": [
    "Keiko I. Nagao"
  ],
  "comment": "3pages, 8 figures. Proceedings for PPAP 2019 (2nd workshop on Phenomenology for Particle and Anti-Particle 2019)",
  "categories": [
    "astro-ph.CO",
    "hep-ex",
    "hep-ph"
  ],
  "abstract": "Velocity distribution of dark matter is supposed to be isotropic Maxwell-Boltzmann distribution in most cases, however, other distribution models including anisotropic one are suggested by simulations. Directional direct detection of dark matter is expected to be a hopeful way to discriminate isotropic distribution from anisotropic one. We investigate the possibility to obtain the anisotropy and WIMP mass by Monte-Carlo simulation supposing the directional detector.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2019-09-19T08:43:06.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "dark matter mass",
      "directional detector",
      "anisotropy",
      "isotropic maxwell-boltzmann distribution",
      "directional direct detection"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 3,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}