Detectability of nontrivial topologies

M. Kunz, N. Aghanim, A. Riazuelo, and O. Forni
Phys. Rev. D 77, 023525 – Published 23 January 2008

Abstract

We study how the uncertainty in the cosmological parameters impacts on the detection of topological signals, focussing on three cubic torus universes and using three tests: the information content, the S/N statistic, and the Bayesian evidence. We find, within the concordance cosmological model, that 3D torus universes with a size of 29Gpc3 or larger cannot be detected. For the toroidal models that can be detected, the detection significance is primarily influenced by ΩΛ, which enters both in the noise amplitude due to the Integrated Sachs-Wolfe effect and in the size of the causal horizon which limits the accessible fundamental domain. On large angular scales <40, only ΩΛ significantly alters the detection for all three estimators considered here.

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  • Received 7 May 2007

DOI:https://doi.org/10.1103/PhysRevD.77.023525

©2008 American Physical Society

Authors & Affiliations

M. Kunz1,*, N. Aghanim2,†, A. Riazuelo3,‡, and O. Forni4,§

  • 1Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland
  • 2IAS, CNRS & Univ. Paris-Sud, Bât. 121, F-91405, Orsay Cedex, France
  • 3Institut d’Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98 bis boulevard Arago, 75014 Paris, France
  • 4CESR, 9 Avenue du Colonel Roche, B.P. 44346, F-31028 Toulouse, Cedex 4, France

  • *Martin.Kunz@physics.unige.ch
  • Nabila.Aghanim@ias.u-psud.fr
  • riazuelo@iap.fr
  • §Olivier.Forni@cesr.fr

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Vol. 77, Iss. 2 — 15 January 2008

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