Running Spectral Index from Large-field Inflation with Modulations Revisited
Michael Czerny, Takeshi Kobayashi, Fuminobu Takahashi
TL;DR
The paper addresses how to reconcile a sizable tensor signal with a suppressed small-scale CMB power by invoking a negative running of the scalar spectral index. It develops a framework of modulated large-field inflation, focusing on multi-natural inflation where multiple sinusoidal terms in the potential can generate a notable running without disrupting overall slow-roll dynamics. The authors show that a negative running compatible with current constraints can arise in a two-sinusoid realization, while also yielding viable predictions for the tensor-to-scalar ratio r. This approach links the B-mode results to microphysical features of the inflaton potential and makes testable predictions for upcoming CMB and gravitational-wave measurements of r, n_s, and the running.
Abstract
We revisit large field inflation models with modulations in light of the recent discovery of the primordial B-mode polarization by the BICEP2 experiment, which, when combined with the Planck + WP + highL data, gives a strong hint for additional suppression of the CMB temperature fluctuations at small scales. Such a suppression can be explained by a running spectral index. In fact, it was pointed out by two of the present authors (TK and FT) that the existence of both tensor mode perturbations and a sizable running of the spectral index is a natural outcome of large inflation models with modulations. We find that this holds also in the recently proposed multi-natural inflation, in which the inflaton potential consists of multiple sinusoidal functions and therefore the modulations are a built-in feature.
