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CMB Constraint on Radion Evolution in the Brane World Scenario
CMB Constraint on Radion Evolution in the Brane World Scenario
2007-06-04
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arxiv.org/abs/0706.0391v2
Phys.Rev.D76:043525,2007
Astronomy and Astrophysics
Astrophysics
7 pages, 6 figures, minor changes of format to conform with PRD
format
Scientific paper
10.1103/PhysRevD.76.043525
In many versions of brane model, the modulus field of extra dimensions, the radion, could have cosmological evolution, which induces variation of the Higgs vacuum expectation value, $$, resulting in cosmological variation of the electron mass $m_e$. The formation of Cosmic Microwave Background (CMB) anisotropies is thus affected, causing changes both in the peaks positions and amplitudes in the CMB power spectra. Using the three-year Wilkinson Microwave Anisotropies Probe (WMAP) CMB data, with the Hubble parameter $H_0$ fixed to be the Hubble Space Telescope (HST) result 72 km s$^{-1}$ Mpc$^{-1}$, we obtain a constraint on $\rho$, the ratio of the value of $$ at CMB recombination to its present value, to be [0.97, 1.02].
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