arXiv · hep-th/0507270
Bouncing Cosmology in Three Dimensions
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.
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Anindya Biswas, Sudipta Mukherji. 2006-01-18. Bouncing Cosmology in Three Dimensions. https://doi.org/10.1088/1475-7516%2F2006%2F02%2F002
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