Scale dependence of in N-flation
arXiv:1009.3326 · doi:10.1088/1475-7516/2010/12/017
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.
15 pages, 2 figures; a subsection with detectable scale dependence of f_NL added; more discussions added and version accepted for publication in JCAP
References in corpus (9)
- Non-Gaussianities in two-field inflation
- Multi-brid inflation and non-Gaussianity
- Scale-dependent non-Gaussianity probes inflationary physics
- Nflation: multi-field inflationary dynamics and perturbations
- Nflation: non-gaussianity in the horizon-crossing approximation
- Scale-dependence of Non-Gaussianity in the Curvaton Model
- On Perturbation Spectra of N-flation
- Negative spectral index of in the axion-type curvaton model
- Weak Gravity Conjecture for the Effective Field Theories with N Species
Cited by in corpus (5)
- A generalized local ansatz and its effect on halo bias
- High-redshift JWST Observations and Primordial Non-Gaussianity
- Testing the Running of non-Gaussianity through the CMB mu-distortion and the Halo Bias
- Scale-Dependent Non-Gaussianity as a Generalization of the Local Model
- Scale and shape dependent non-Gaussianity in the presence of inflationary vector fields