Fig. 2.

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Maximum correlation angle due to inflation. Top panel (a): 3D plot of the maximum correlation angle as a function of cosmic time and the number of e-folds. Bottom panel (b): maximum correlation angle evolution with cosmic time for different Ne values, corresponding to vertical sections in the 3D plot. We highlight that the plateau for Ne is smaller than about 50, implying a large inhomogeneity of the CMB along cosmic time.
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