51. Dark coupling
- Author
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Gavela, M. B., Hernandez, D., Honorez, L. Lopez, Mena, O., and Rigolin, S.
- Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics ,High Energy Physics - Phenomenology - Abstract
The two dark sectors of the universe - dark matter and dark energy - may interact with each other. Background and linear density perturbation evolution equations are developed for a generic coupling. We then establish the general conditions necessary to obtain models free from early time non-adiabatic instabilities. As an application, we consider a viable universe in which the interaction strength is proportional to the dark energy density. The scenario does not exhibit "phantom crossing" and is free from instabilities, including early ones. A sizeable interaction strength is compatible with combined WMAP, HST, SN, LSS and H(z) data. Neutrino mass and/or cosmic curvature are allowed to be larger than in non-interacting models. Our analysis sheds light as well on unstable scenarios previously proposed., Comment: 30 pages, 10 figures
- Published
- 2009
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