Theoriekolloquium
Nov. 29, 2012 at 3:30 p.m. in Newton-Raum, Staudinger Weg 9, 01-122Prof. Dr. P.G.J. van Dongen
Institut für Physik, KOMET 7
peter.vandongen@uni-mainz.de
Jun.-Prof. Dr. J. Marino
Institut für Physik, KOMET 7
jamarino@uni-mainz.de
In any approach to quantum gravity, it is crucial to look for observational effects. In my talk, I discuss how quantum gravitational contributions to the anisotropy spectrum of the cosmic microwave background arise in the framework of quantum geometrodynamics (Wheeler-DeWitt equation). From the present non-observation of these contributions, we find a constraint on the Hubble parameter of inflation. I also compare these results with the predictions from loop quantum cosmology.