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arxiv: 1405.0734 · v2 · pith:I3EZ76X6new · submitted 2014-05-04 · ✦ hep-th · astro-ph.CO· hep-ph

Notes on natural inflation

classification ✦ hep-th astro-ph.COhep-ph
keywords axion-likeinflationinflatonlargeconstantdecaylimitnatural
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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 ${\mathcal N}=1$ Super-Yang-Mills which allows us to treat finite N. This analysis also suggests that moderately large gauge groups such as $E_{8}$ are good enough with a Planck scale decay constant.

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