{
  "id": "astro-ph/9812328",
  "version": "v1",
  "published": "1998-12-17T14:52:59.000Z",
  "updated": "1998-12-17T14:52:59.000Z",
  "title": "MOND in the Early Universe",
  "authors": [
    "Stacy McGaugh"
  ],
  "comment": "Contribution to '98 October conference, After the Dark Ages, eds. Smith & Holt, 4 pages",
  "doi": "10.1063/1.58637",
  "categories": [
    "astro-ph",
    "gr-qc",
    "hep-ph"
  ],
  "abstract": "I explore some consequences of Milgrom's modified dynamics for cosmology. There appear to be two promising tests for distinguishing MOND from CDM: (1) the rate of growth of structure and (2) the baryon fraction. These should be testable with observations of clusters at high redshift and the microwave background, respectively.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1998-12-17T14:52:59.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "early universe",
      "milgroms modified dynamics",
      "baryon fraction",
      "high redshift",
      "microwave background"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 491527
    }
  }
}