The Cosmological Slingshot Scenario

by Dr Cristiano Germani (SISSA)

Wednesday 7 Nov 2007, 11:00 → 12:00 Europe/Zurich

1/1-025 (CERN)

I will discuss a new cosmological model for the early time Universe. In this model, the Universe is a wandering brane moving in a warped throat of a Calabi-Yau space. A non-zero angular momentum induces a turning point in the brane trajectory, and leads to a bouncing cosmology as experienced by an observer living on the brane. The Universe undergoes a decelerated contraction followed by an accelerating expansion and no big-bang singularity. Although the number of e-folds of accelerated motion is low (less than 2), standard cosmological problems are not present in the slingshot thanks to the absence of an initial singularity and the violation of energy conditions of mirage matter at high energies. Density perturbations are also calculated and a slightly red spectral index with negligible tensorial perturbations is found in compatibility with WMAP data. I will base my presentation on arXiv:0706.0025 arXiv:0706.0023 hep-th/0611246