{
  "id": "1606.03843",
  "version": "v1",
  "published": "2016-06-13T07:25:10.000Z",
  "updated": "2016-06-13T07:25:10.000Z",
  "title": "Pulsars as probes of gravity and fundamental physics",
  "authors": [
    "Michael Kramer"
  ],
  "comment": "22 pages, 1 figures, in Proceedings of 14th Marcel-Grossmann Meeting, to appear in IJMPD",
  "categories": [
    "astro-ph.HE",
    "gr-qc"
  ],
  "abstract": "Radio-loud neutron stars known as pulsars allow a wide range of experimental tests for fundamental physics, ranging from the study of super-dense matter to tests of general relativity and its alternatives. As a result, pulsars provide strong-field tests of gravity, they allow for the direct detection of gravitational waves in a 'pulsar timing array', and they promise the future study of black hole properties. This contribution gives an overview of the on-going experiments and recent results.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-06-13T07:25:10.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "fundamental physics",
      "radio-loud neutron stars",
      "black hole properties",
      "general relativity",
      "strong-field tests"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 22,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}