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String theory clues for the low–ℓ CMB ?

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Figure

Figure 1. τlines forconformal time–evolution of the scalar field near the turning point (left), the corresponding MS potentials Ws in η (center) and an enlarged view of the region where the Ws cross the horizontal axis (right)
Figure 2. Power spectra of scalar perturbations for the double–exponential potential of eq
Figure 4. The eof theffect of a slightly negative γ in the two–exponential potential. We focus on a smaller portion k that is still realistic with these models, and yet suffices to get fair χ2 estimates
Figure 6. WMAP9 determination [21] of the CMB angular power spectrum (left), the raw data for its low–ℓportion (center) and the corresponding PLANCK determination [20] (right)
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