DBI models for the unification of dark matter and dark energy
arXiv:0904.1114 · doi:10.1007/s10714-009-0901-z
Abstract
We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution of perturbations. We also perform a Bayesian analysis to set observational constraints on the parameters of the model using type Ia SN, CMB shift and BAO data. Finally, to complete the study we investigate its kinematics aspects, such as the effective equation of state parameter, acceleration parameter and transition redshift. Particularizing those parameters for the best fit one appreciates that an effective phantom is preferred.
11 pages, 8 figures, revtex, new references
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Cited by in corpus (13)
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- Analysing dissipative effects in the CDM model
- Reduced modified Chaplygin gas cosmology
- CMB-Galaxy correlation in Unified Dark Matter Scalar Field Cosmologies
- Raychaudhuri equation in -essence geometry: conditional singular and non-singular cosmological models
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