{
  "id": "astro-ph/9512155",
  "version": "v1",
  "published": "1995-12-22T22:29:28.000Z",
  "updated": "1995-12-22T22:29:28.000Z",
  "title": "Dependence of Inflationary Reconstruction upon Cosmological Parameters",
  "authors": [
    "Michael Turner",
    "Martin White"
  ],
  "comment": "15 pages, LaTeX, 3 postscript figures (included with epsf), submitted to Phys. Rev. D",
  "journal": "Phys.Rev.D53:6822-6828,1996",
  "doi": "10.1103/PhysRevD.53.6822",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The inflationary potential and its derivatives determine the spectrum of scalar and tensor metric perturbations that arise from quantum fluctuations during inflation. The CBR anisotropy offers a promising means of determining the spectra of metric perturbations and thereby a means of constraining the inflationary potential. The relation between the metric perturbations and CBR anisotropy depends upon cosmological parameters -- most notably the possibility of a cosmological constant. Motivated by some observational evidence for a cosmological constant (large-scale structure, cluster-baryon fraction, measurements of the Hubble constant and age of the Universe) we derive the reconstruction equations and consistency relation to second order in the presence of a cosmological constant. We also clarify previous notation and discuss alternative schemes for reconstruction.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1995-12-22T22:29:28.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "98.70.Vc",
      "98.80.Cq"
    ],
    "keywords": [
      "cosmological parameters",
      "inflationary reconstruction",
      "cosmological constant",
      "dependence",
      "inflationary potential"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Phys. Rev. D"
    },
    "note": {
      "typesetting": "LaTeX",
      "pages": 15,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 404078
    }
  }
}