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Bouncing Cosmology in Three Dimensions

arXiv:hep-th/0507270 · doi:10.1088/1475-7516/2006/02/002

Abstract

We consider a dynamical two-brane in a four dimensional black hole background with scalar hair. At high temperature this black hole goes through a phase transition by radiating away the scalar. The end phase is a topological adS-Schwarzschild black hole. We argue here that for a sufficiently low temperature, the brane motion in this geometry is non-singular. This results in a universe which passes over from a contracting phase to an expanding one without reaching a singularity.

7 pages, LaTex, 3 figures, Journal version

Bouncing Cosmology in Three Dimensions · wovepaper