The spectral index and its running in axionic curvaton
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 dns/dln k ~ 2π/ΔN (ns-1), where ΔN 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.
- Publication:
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Journal of Cosmology and Astroparticle Physics
- Pub Date:
- June 2013
- DOI:
- arXiv:
- arXiv:1301.2834
- Bibcode:
- 2013JCAP...06..013T
- Keywords:
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- Astrophysics - Cosmology and Extragalactic Astrophysics;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- E-Print:
- 17 pages, 2 figrues