Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-06-25
Phys.Rev. D62 (2000) 087304
Astronomy and Astrophysics
Astrophysics
4 pages, RevTeX, 7 Figures
Scientific paper
10.1103/PhysRevD.62.087304
The cosmic microwave background radiation allows us to measure both the geometry and topology of the universe. It has been argued that the COBE-DMR data already rule out models that are multiply connected on scales smaller than the particle horizon. Here we show the opposite is true: compact (small) hyperbolic universes are favoured over their infinite counterparts. For a density parameter of Omega_o=0.3, the compact models are a better fit to COBE-DMR (relative likelihood ~20) and the large-scale structure data (sigma_8 increases by ~25%).
Cornish Neil J.
Spergel David N.
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