4.6 Article

The spectral index and its running in axionic curvaton

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2013/06/013

Keywords

physics of the early universe; cosmological parameters from CMBR; cosmology of theories beyond the SM; cosmological perturbation theory

Funding

  1. World Premier International Center Initiative (WPI Program), MEXT, Japan
  2. [24111702]
  3. [21111006]
  4. [23104008]
  5. [22244030]
  6. [21244033]
  7. [24740135]
  8. Grants-in-Aid for Scientific Research [22244030] Funding Source: KAKEN

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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 dn(s)/dln k similar to 2 pi/Delta N(n(s) - 1), where Delta N 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.

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