1993/05/23 by A. A. Starobinsky
Physics and Astronomy · #gr-qc #astro-ph
published as JETP Lett. 57 (1993) 622-625 · 4 pages, report LANDAU-93-04/GR-1
arxiv created 1993/05/23 · arxiv updated 2009/11/30
If the Universe has the topology of a 3-torus (T3), then it follows from recent data on large-scale temperature fluctuations ΔT/T of the cosmic microwave background that either the minimal size of the torus is at least of the order of the present cosmological horizon, or the large-scale ΔT/T pattern should have a symmetry plane (in case of the effective T1 topology) or a symmetry axis (in case of the effective T2 topology), the latter possibility being probably excluded by the data.