A Field Theory Model for Dark Matter and Dark Energy in Interaction
arXiv:0902.0318 · doi:10.1103/PhysRevD.79.123506
Abstract
We propose a field theory model for dark energy and dark matter in interaction. Comparing the classical solutions of the field equations with the observations of the CMB shift parameter, BAO, lookback time and Gold supernovae sample, we observe a possible interaction between dark sectors with energy decay from dark energy into dark matter. The observed interaction provides an alleviation to the coincidence problem.
15 pages, 9 figures; references added; new conclusions drawn from new figures and computations
References in corpus (8)
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Constraining Interactions in Cosmology's Dark Sector
- Observational constraints on the dark energy and dark matter mutual coupling
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- Reconstruction of interacting dark energy models from parameterizations
- The mass and the coupling of the Dark Particle