Dark Energy and Dark Matter unification via superfluid Chaplygin gas
arXiv:0912.1609 · doi:10.1016/j.physletb.2010.02.035
Abstract
A new model describing the dark sector of the universe is established. The model involves Bose-Einstein condensate (BEC) as dark energy (DE) and an excited state above it as dark matter (DM). The condensate is assumed to have a negative pressure and is embodied as an exotic fluid with Chaplygin equation of state. Excitations are described as a quasiparticle gas. It is shown that the model is not in disagreement with the current observations of the cosmic acceleration. The model predicts increase of the effective cosmological constant and a complete disappearance of the matter at the far future.
13 pages, 3 figures
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- Large-scale structure in superfluid Chaplygin gas cosmology
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- Statefinder analysis of the superfluid Chaplygin gas model
- The Formulation of Scaling Expansion in an Euler-Poisson Dark-fluid Model
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