Constraining the Topology of the Universe

Neil J. Cornish, David N. Spergel, Glenn D. Starkman, and Eiichiro Komatsu
Phys. Rev. Lett. 92, 201302 – Published 19 May 2004

Abstract

The first year data from the Wilkinson Microwave Anisotropy Probe are used to place stringent constraints on the topology of the Universe. We search for pairs of circles on the sky with similar temperature patterns along each circle. We restrict the search to back-to-back circle pairs, and to nearly back-to-back circle pairs, as this covers the majority of the topologies that one might hope to detect in a nearly flat universe. We do not find any matched circles with radius greater than 25°. For a wide class of models, the nondetection rules out the possibility that we live in a universe with topology scale smaller than 24 Gpc.

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  • Received 8 October 2003

DOI:https://doi.org/10.1103/PhysRevLett.92.201302

©2004 American Physical Society

Authors & Affiliations

Neil J. Cornish1, David N. Spergel2, Glenn D. Starkman3,4, and Eiichiro Komatsu2,5

  • 1Department of Physics, Montana State University, Bozeman, Montana 59717, USA
  • 2Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA
  • 3Center for Education and Research in Cosmology and Astrophysics, Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106-7079, USA
  • 4CERN Theory Division, CH-1211 Geneva 23, Switzerland
  • 5Department of Astronomy, The University of Texas at Austin, Austin, Texas 78712, USA

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Issue

Vol. 92, Iss. 20 — 21 May 2004

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