Abstract

We investigate the possible implications of the measured value of the scalar tilt nsn_s for the tensor-to-scalar ratio rr in slow-roll, single-field inflationary models. The measured value of the tilt satisfies ns−1∼1/N∗n_s -1\sim 1/N_*, where N∗∼60N_* \sim 60 is the number of ee-folds for observationally relevant scales. If this is not a coincidence and the scaling holds for different values of NN, it strongly suggests that either rr is as big as 10−110^{-1} (a possibility in tension with the recent data), or smaller than 10−210^{-2} and exponentially dependent on nsn_s. A large region of the (nsn_s,rr) plane is not compatible with this scaling.

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