Abstract
A class of braneworld models can lead to phantom-like acceleration of the late universe, but without the need for any phantom matter. In the simplest models, the universe contains only cold dark matter and a cosmological constant. We generalize these models by introducing a quintessence field. The new feature in our models is that quintessence leads to a crossing of the phantom divide, w = −1. This is a purely gravitational effect, and there is no phantom instability. Furthermore, the Hubble parameter is always decreasing, and there is no big rip singularity in the future
Original language | English |
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Pages (from-to) | 004-004 |
Number of pages | 1 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2006 |
Issue number | 09 |
DOIs | |
Publication status | Published - 2006 |