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The Topology and Size of the Universe from the Cosmic Microwave Background (1104.0015v2)
Published 31 Mar 2011 in astro-ph.CO, hep-ph, and hep-th
Abstract: We study the possibility that the universe has compact topologies T3, T2 x R1, or S1 x R2 using the seven-year WMAP data. The maximum likelihood 95% confidence intervals for the size L of the compact direction are 1.7 < L/L_0 < 2.1, 1.8 < L/L_0 < 2.0, 1.2 < L/L_0 < 2.1 for the three cases, respectively, where L_0=14.4 Gpc is the distance to the last scattering surface. An infinite universe is compatible with the data at 4.3 sigma. We find using a Bayesian analysis that the most probable universe has topology T2 x R1, with L/L_0=1.9.