Curvaton potential terms, scale-dependent perturbation spectra and chaotic initial conditions
Abstract
The curvaton scenario predicts an almost scale-invariant spectrum of perturbations in most inflation models. We consider the possibility that renormalizable phi4 or Planck scale-suppressed non-renormalizable curvaton potential terms may result in an observable deviation from scale-invariance. We show that if the curvaton initially has a large amplitude and if the total number of e-foldings of inflation is less than about 300 then a running blue perturbation spectrum with an observable deviation from scale-invariance is likely. D-term inflation is considered as an example with a potentially low total number of e-foldings of inflation. A secondary role for the curvaton, in which it drives a period of chaotic inflation leading to D-term or other flat potential inflation from an initially chaotic state, is suggested.
- Publication:
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Journal of Cosmology and Astroparticle Physics
- Pub Date:
- December 2003
- DOI:
- 10.1088/1475-7516/2003/12/005
- arXiv:
- arXiv:hep-ph/0308295
- Bibcode:
- 2003JCAP...12..005M
- Keywords:
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- High Energy Physics - Phenomenology
- E-Print:
- 12 pages LaTeX, minor corrections, to be published in JCAP