Notes on natural inflation
arXiv:1405.0734 · doi:10.1088/1475-7516/2014/10/054
Abstract
In the so-called natural inflation, an axion-like inflaton is assumed to have a cosine-type periodic potential. This is not the case in a very simple model in which the axion-like inflaton is coupled to an SU(N) (or other) pure Yang-Mills, at least in the large N limit as pointed out by Witten. It has a multi-valued potential, which is effectively quadratic, i.e., there is only a mass term in the large N limit. Thanks to this property, chaotic inflation can be realized more naturally with the decay constant of the axion-like inflaton less than the Planck scale. We demonstrate these points explicitly by using softly broken Super-Yang-Mills which allows us to treat finite N. This analysis also suggests that moderately large gauge groups such as are good enough with a Planck scale decay constant.
12 pages. v2: Published version
References in corpus (9)
- Monodromy in the CMB: Gravity Waves and String Inflation
- A Natural Framework for Chaotic Inflation
- An Ignoble Approach to Large Field Inflation
- Natural Chaotic Inflation and UV Sensitivity
- or Not : Testing the Simplest Inflationary Potential
- Dynamical Chaotic Inflation in the Light of BICEP2
- Simple realization of inflaton potential on a Riemann surface
- Grand Unification, Axion, and Inflation in Intermediate Scale Supersymmetry
- Monodromy Inflation in SUSY QCD
Cited by in corpus (8)
- Natural Inflation and Quantum Gravity
- Axion Monodromy Inflation on Warped Throats
- Axion Landscape and Natural Inflation
- Modified Lyth bound and implications of BICEP2 results
- Dynamical Fractional Chaotic Inflation -- Dynamical Generation of a Fractional Power-Law Potential for Chaotic Inflation
- Natural Braneworld Inflation in Light of Recent Results from Planck and BICEP2
- Phase Locked Inflation -- Effectively Trans-Planckian Natural Inflation
- A keV String Axion from High Scale Supersymmetry