Cosmological Effects of Radion Oscillations

L. Perivolaropoulos; C. Sourdis

doi:10.1103/PhysRevD.66.084018

paper

Cosmological Effects of Radion Oscillations

arXiv:hep-ph/0204155 · doi:10.1103/PhysRevD.66.084018

Abstract

We show that the redshift of pressureless matter density due to the expansion of the universe generically induces small oscillations in the stabilized radius of extra dimensions (the radion field). The frequency of these oscillations is proportional to the mass of the radion and can have interesting cosmological consequences. For very low radion masses $m_{b}$ ( $m_{b} \sim 10 - 100 H_{0} ≃ 1 0^{- 32} e V$ ) these low frequency oscillations lead to oscillations in the expansion rate of the universe. The occurrence of acceleration periods could naturally lead to a resolution of the coincidence problem, without need of dark energy. Even though this scenario for low radion mass is consistent with several observational tests it has difficulty to meet fifth force constraints. If viewed as an effective Brans-Dicke theory it predicts $ω = - 1 + \frac{1}{D}$ ( $D$ is the number of extra dimensions), while experiments on scales larger than $1 mm$ imply $ω > 2500$ . By deriving the generalized Newtonian potential corresponding to a massive toroidally compact radion we demonstrate that Newtonian gravity is modified only on scales smaller than $m_{b}^{- 1}$ . Thus, these constraints do not apply for $m_{b} > 1 0^{- 3} e V$ (high frequency oscillations) corresponding to scales less than the current experiments ( $0.3 mm$ ). Even though these high frequency oscillations can not resolve the coincidence problem they provide a natural mechanism for dark matter generation. This type of dark matter has many similarities with the axion.

Accepted in Phys. Rev. D. Clarifying comments added in the text and some additional references included

Cosmological Effects of Radion Oscillations

Abstract

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