{
  "id": "0912.0384",
  "version": "v1",
  "published": "2009-12-02T10:16:35.000Z",
  "updated": "2009-12-02T10:16:35.000Z",
  "title": "Gravitational waves from neutron stars: Promises and challenges",
  "authors": [
    "N. Andersson",
    "V. Ferrari",
    "D. I. Jones",
    "K. D. Kokkotas",
    "B. Krishnan",
    "J. Read",
    "L. Rezzolla",
    "B. Zink"
  ],
  "comment": "review article for Einstein Telescope special issue in Gen Rel Grav, 39 pages, 7 figures",
  "journal": "Gen.Rel.Grav.43:409-436,2011",
  "doi": "10.1007/s10714-010-1059-4",
  "categories": [
    "astro-ph.SR",
    "astro-ph.HE",
    "gr-qc"
  ],
  "abstract": "We discuss different ways that neutron stars can generate gravitational waves, describe recent improvements in modelling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to test our understanding of fundamental physics. The main purpose of the discussion is to establish promising science goals for third-generation ground-based detectors, like the Einstein Telescope, and identify the various challenges that need to be met if we want to use gravitational-wave data to probe neutron star physics.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-12-02T10:16:35.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "challenges",
      "probe neutron star physics",
      "generate gravitational waves",
      "improving detector sensitivity",
      "gravitational-wave data"
    ],
    "tags": [
      "review article",
      "journal article"
    ],
    "publication": {
      "journal": "General Relativity and Gravitation",
      "year": 2011,
      "month": "Feb",
      "volume": 43,
      "number": 2,
      "pages": 409
    },
    "note": {
      "typesetting": "TeX",
      "pages": 39,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 838776,
      "adsabs": "2011GReGr..43..409A"
    }
  }
}