Quintom dark energy in DGP braneworld cosmology

Details Quintom dark energy in DGP braneworld cosmology Quintom dark energy in DGP braneworld cosmology

2008-06-15

arxiv.org/abs/0806.2418v2

Phys. Lett. B 674, 237, (2009)

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages, 8 figures

Scientific paper

10.1016/j.physletb.2009.03.051

In this paper we consider a $Z_2$ 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 $\epsilon=1$, and an asymptotically static universe in negative branch $\epsilon=-1$.

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