In the Cosmological Slingshot Scenario, our Universe is a D3-brane that
extends in the 4d noncompact directions of a warped Calabi-Yau compactification
of IIB Supergravity. Early time cosmology corresponds to a period in which the
brane moves inside a warped throat where a non-vanishing angular momentum
ensures that the trajectory of the brane has a turning point. The corresponding
induced metric on the D3-brane experiences a cosmological evolution with a
bounce. In this framework, the homogeneity, flatness, and isotropy problems of
standard cosmology might be avoided. The power spectrum of primordial
perturbations of the brane embedding can be found and it is shown to be in
agreement to WMAP data.Comment: Presented at "Ten Years of AdS/CFT: A Workshop Celebrating the Tenth
Anniversary of the Maldacena Conjecture", Buenos Aires, Argentina, 19-21 Dec
200