Freiburg 2008 – scientific programme
Parts | Days | Selection | Search | Downloads | Help
GR: Fachverband Gravitation und Relativitätstheorie
GR 1: Kosmologie
GR 1.2: Talk
Monday, March 3, 2008, 17:05–17:25, KGI-HS 1010
Cosmic Topology and Cosmic Microwave Background (CMB) — •Sven Lustig — Universität Ulm, Institut für Theoretische Physik, Albert-Einstein-Allee 11, D-89069 Ulm
How well can the topology of our Universe be constrained by the WMAP data? This question shall be dicussed on the basis of the angular power spectrum of the CMB and the so-called "circle-in-the-sky" signature.