Supersymmetron
arXiv:1109.0468 · doi:10.1016/j.physletb.2011.11.060
Abstract
We consider a supersymmetric model of dark energy coupled to cold dark matter: the supersymmetron. In the absence of cold dark matter, the supersymmetron converges to a supersymmetric minimum with a vanishing cosmological constant. When cold dark matter is present, the supersymmetron evolves to a matter dependent minimum where its energy density does not vanish. In the early universe until the recent past of the Universe, the energy density of the supersymmetron is negligible compared to the cold dark matter energy density. Away from the supersymmetric minimum, the equation of state of the supersymmetron is constant and negative. When the supersymmetron reaches the neighbourhood of the supersymmetric minimum, its equation of state vanishes rapidly. This leads to an acceleration of the universe which is transient unless supersymmetry breaking induces a pure cosmological constant and acceleration of the Universe does not end. Moreover, we find that the mass of supersymmetron is always greater than the gravitino mass. As a result, the supersymmetron generates a short ranged fifth force which evades gravitational tests. On the other hand, we find that the supersymmetron may lead to relevant effects on large scale structures.
published version, 11 pages
References in corpus (8)
- Dynamics of dark energy
- Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
- Environmental Dependence of Masses and Coupling Constants
- The Dilaton and Modified Gravity
- Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory
- Constraining Interactions in Cosmology's Dark Sector
- Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
- New interactions in the dark sector mediated by dark energy
Cited by in corpus (10)
- Beyond the Cosmological Standard Model
- Chameleon Field Theories
- Disformal Gravity Theories: A Jordan Frame Analysis
- Screening the fifth force in the Horndeski's most general scalar-tensor theories
- Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
- Dynamics of Supersymmetric Chameleons
- SUPER-Screening
- Chameleonic inflation
- Chameleonic Theories: A Short Review
- The Cosmological Supersymmetron