arXiv:1009.3326·v3·Cosmology and Nongalactic Astrophysics
Scale dependence of in N-flation
Abstract
Adopting the horizon-crossing approximation, we derive the spectral index of in general N-flation model. Axion N-flation model is taken as a typical model for generating a large which characterizes the size of local form bispectrum. We find that its tilt is negligibly small when all inflatons have the same potential, but a negative detectable can be achieved in the axion N-flation with different decay constants for different inflatons. The measurement of can be used to support or falsify the axion N-flation in the near future.
Comments: 15 pages, 2 figures; a subsection with detectable scale dependence of f_NL added; more discussions added and version accepted for publication in JCAP