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20052010201520202023051015
Abstract: (arXiv)
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=1w=-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.
  • membrane model
  • expansion: acceleration
  • quintessence
  • Dvali-Gabadadze-Porrati model
  • dynamical system
  • phantom