Cosmology from Moduli Dynamics
arXiv:hep-th/0407063 · doi:10.1088/1126-6708/2004/08/053
Abstract
We investigate moduli field dynamics in supergravity/M-theory like set ups where we turn on fluxes along some or all of the extra dimensions. As has been argued in the context of string theory, we observe that the fluxes tend to stabilize the squashing (or shape) modes. Generically we find that at late times the shape is frozen while the radion evolves as a quintessence field. At earlier times we have a phase of radiation domination where both the volume and the shape moduli are slowly evolving. However, depending on the initial conditions and the parameters of the theory, like the value of the fluxes, curvature of the internal manifold and so on, the dynamics of the internal manifold can be richer with interesting cosmological consequences, including inflation.
38 pages, 6 figures; references added
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Cited by in corpus (12)
- Moduli Stabilization in Brane Gas Cosmology with Superpotentials
- AdS and stabilized extra dimensions in multidimensional gravitational models with nonlinear scalar curvature terms 1/R and R^4
- Deviations From Newton's Law in Supersymmetric Large Extra Dimensions
- UV Sensitivity in Supersymmetric Large Extra Dimensions: The Ricci-flat Case
- Coupled Inflation and Brane Gases
- Current Acceleration from Dilaton and Stringy Cold Dark Matter
- Trapped Quintessential Inflation in the context of Flux Compactifications
- Cyclic Inflation
- MSLED, Neutrino Oscillations and the Cosmological Constant
- Scaling solutions and geodesics in moduli space
- The dynamics of coset dimensional reduction
- Dark energy in hybrid inflation