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Cosmological Avatars of the Landscape II CMB and LSS Signatures.pdf

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Figure

FIG. 1: CMB TT power spectra for the cases with b = 4.0 × 10 9 GeV (dash-line) and 3.8×10 9 GeV (dot-line)
FIG. 2: Matter power spectra for the same values of b as Fig.1, described in Section III
Fig. 3 shows our results for this cross-correlation. In the fig- fig-ure, we take b = 4.0 × 10 9 and 3.6 × 10 9 GeV as an example.
FIG. 4: The same as Fig.3 except we plotted the larger range of mul- mul-tipoles here.

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