Fractional contribution of isocurvature modes to the power spectrum. We show the distributions αℐℐ(2,20), αℛℐ(2,20), αℐℐ(21,200), αℛℐ(21,200), αℐℐ(201,2500), and αℛℐ(201,2500), defined in Eq. (69), for the CDI, NDI, and NVI modes as constrained by the Planck+WP data.
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