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arxiv: 1105.0073 · v2 · pith:A6RRKHGJnew · submitted 2011-04-30 · ✦ hep-ph · astro-ph.CO· gr-qc· hep-th

Large non-Gaussianity in non-minimal inflation

classification ✦ hep-ph astro-ph.COgr-qchep-th
keywords inflationangulardirectionbecomescomplexlargemodelmodulus
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We consider a simple inflation model with a complex scalar field coupled to gravity non-minimally. Both the modulus and the angular directions of the complex scalar are slowly rolling, leading to two-field inflation. The modulus direction becomes flat due to the non-minimal coupling, and the angular direction becomes a pseudo-Goldstone boson from a small breaking of the global U(1) symmetry. We show that large non-Gaussianity can be produced during slow-roll inflation under a reasonable assumption on the initial condition of the angular direction. This scenario may be realized in particle physics models such as the Standard Model with two Higgs doublets.

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