The Spectral Index and its Running in Axionic Curvaton
Fuminobu Takahashi
TL;DR
The paper addresses whether a sizable running of the scalar spectral index can be explained in a curvaton scenario rather than single-field inflation. It introduces an axionic curvaton with a potential comprising two sinusoidal terms, leading to oscillations of $n_s-1$ and $\alpha$ as the curvaton evolves, with a generic relation $\alpha \sim \frac{2\pi}{\Delta N}(n_s-1)$. Matching the SPT/WMAP pivot data requires $\Delta N$ of order $20$–$30$ e-folds per modulation, and the model can reproduce the observed negative running $\alpha \approx -0.024$ at the SPT pivot. The mechanism draws support from the string axiverse, where axions obtain masses from multiple instanton contributions, and it remains compatible with red-tilted spectra with negligible running for suitable $\Delta N$, offering a simple, non-large-field inflation realization.
Abstract
We show that a sizable running spectral index suggested by the recent SPT data can be explained in the axionic curvaton model with a potential that consists of two sinusoidal contributions of different height and period. We find that the running spectral index is generically given by d ns/dlnk ~ (2pi/dN)(n_s - 1), where dN is the e-folds during one period of modulations. In the string axiverse, axions naturally acquire a mass from multiple contributions, and one of the axions may be responsible for the density perturbations with a sizable running spectral index via the curvaton mechanism. We note that the axionic curvaton model with modulations can also accommodate the red-tilted spectrum with a negligible running, without relying on large-field inflation.
