{
  "id": "astro-ph/0007204",
  "version": "v1",
  "published": "2000-07-14T19:24:57.000Z",
  "updated": "2000-07-14T19:24:57.000Z",
  "title": "Placing limits on the spin-torsion fluctuation from the stability of Friedmann solution and COBE data",
  "authors": [
    "L. C. Garcia de Andrade"
  ],
  "comment": "Latex file",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The gravitational stability of Friedmann metric with respect to homogeneous and isotropic perturbations in Einstein-Cartan cosmology is used together with the COBE data to place a limit on the spin-torsion primordial density fluctuation.Cosmological perturbations in Bianchi type III models are shown to have no contributions from torsion at the early stages of the Universe.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2000-07-14T19:24:57.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cobe data",
      "spin-torsion fluctuation",
      "friedmann solution",
      "placing limits",
      "spin-torsion primordial density fluctuation"
    ],
    "note": {
      "typesetting": "LaTeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 546674,
      "adsabs": "2000astro.ph..7204G"
    }
  }
}