Quintom dark energy in DGP braneworld cosmology
arXiv:0806.2418 · doi:10.1016/j.physletb.2009.03.051
Abstract
In this paper we consider a symmetrical 3-brane embedded in a 5-dimensional spacetime. We study the effective Einstein equation and acceleration condition in presence of the quintom dark energy fluid as the bulk matter field. It is shown that the time-dependent bulk quintom field induces a time-dependent cosmological constant on the brane. In the framework of the DGP model, the effective Einstein equation is obtained in two different cases: i) where the quintom field is considered as the bulk matter field and the brane is empty and, ii) where the quintom dark energy is confined on the brane and the bulk is empty. We show that in both cases one could obtain a self-inflationary solution at late time in positive branch , and an asymptotically static universe in negative branch .
12 pages, 8 figures
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- Restoring New Agegraphic Dark Energy in RS II Braneworld
- Brane-Bulk energy exchange and agegraphic dark energy
- Stability analysis of the cosmological solutions with induced gravity and scalar field on the brane
- Crossing the Cosmological Constant Line on a Warped DGP Brane
- Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
- Quintom wormholes
- Constant-roll Inflation in Brane Induced Gravity Cosmology
- Bulk scalar field in brane-worlds with induced gravity inspired by the term
- Dynamics of the universe as a "test 3-brane" in a 5D bulk
- CDM, DGP and extended phantom-like cosmologies