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
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- Exact black hole solution with a minimally coupled scalar field
- Mirage Cosmology
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Cited by in corpus (11)
- Topological black holes dressed with a conformally coupled scalar field and electric charge
- Electrically charged black hole with scalar hair
- A classical bounce: constraints and consequences
- Static black hole solutions with a self interacting conformally coupled scalar field
- A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
- Dynamic domain walls in Maxwell-Dilaton background
- Domain walls in Born-Infeld-dilaton background
- Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
- Loop quantum cosmology in 2+1 dimension
- Semi-realistic Bouncing Domain Wall Cosmology
- 2+1 dimensional loop quantum cosmology of Bianchi I models