Observational constraints on the dark energy and dark matter mutual coupling
arXiv:0804.0110 · doi:10.1016/j.physletb.2008.05.066
Abstract
We examine different phenomenological interaction models for Dark Energy and Dark Matter by performing statistical joint analysis with observational data arising from the 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy Probe observations, the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey and age estimates of 35 galaxies. Including the time-dependent observable, we add sensitivity of measurement and give complementary results for the fitting. The compatibility among three different data sets seem to imply that the coupling between dark energy and dark matter is a small positive value, which satisfies the requirement to solve the coincidence problem and the second law of thermodynamics, being compatible with previous estimates.
9 pages, 4 figures, accepted for publication in Phys. Lett. B
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Cited by in corpus (7)
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Effects of dark sectors' mutual interaction on the growth of structures
- A Field Theory Model for Dark Matter and Dark Energy in Interaction
- Dynamics of interacting dark energy model in Einstein and Loop Quantum Cosmology
- Constraints on coupling constant between dark energy and dark matter
- A preliminary analysis of the energy transfer between the dark sectors of the Universe
- Crossing the phantom divide line in the Holographic dark energy model in a closed universe