{
  "id": "1305.6549",
  "version": "v1",
  "published": "2013-05-28T16:15:26.000Z",
  "updated": "2013-05-28T16:15:26.000Z",
  "title": "Application of the 3-space approach to the Bianchi II cosmological model",
  "authors": [
    "Lau Loi So"
  ],
  "comment": "5 pages",
  "categories": [
    "gr-qc"
  ],
  "abstract": "Einstein used 4-dimensional space time geometry to explain gravity. However, in 1962, Baierlein, Sharp and Wheeler proposed a Jacobi type timeless Lagrangian based on the 3-dimensional geometry of space to reproduce the same physics. In 2002, Barbour $et$. $al$. further extended this idea and they call it 3-space approach. Here we use Bianchi II cosmological model to demonstrate the 3-space idea. Indeed, we find that this theory is more fundamental and the manipulation is more practical. We recover the known and find a new solutions.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-05-28T16:15:26.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cosmological model",
      "application",
      "space time geometry",
      "jacobi type timeless lagrangian",
      "explain gravity"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1235725,
      "adsabs": "2013arXiv1305.6549L"
    }
  }
}