Chaplygin DGP cosmologies

Details Chaplygin DGP cosmologies Chaplygin DGP cosmologies

2007-06-26

arxiv.org/abs/0706.3896v1

Phys.Lett.B654:51-57,2007

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, revtex

Scientific paper

10.1016/j.physletb.2007.07.063

A new class of braneworld models displaying late-time phantom acceleration without resorting to a phantom fluid is presented. In this scenario expansion is fuelled by dark matter together with some effective dark energy capable of crossing the phantom divide. Unlike a previous proposal of this nature, in these models the effective phantom behaviour remains valid at all redshifts for some choices of the free parameters of the models. The construction is based on the generalised Chaplygin gas, and the cosmological history interpolates between a standard CDM-like behaviour at early times and a de Sitter-like behaviour at late times, so no future singularity is reached.

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