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Helical Phase Inflation

Published 10 Sep 2014 in hep-th, astro-ph.CO, and hep-ph | (1409.3267v2)

Abstract: We show that the quadratic inflation can be realized by the phase of a complex field with helicoid potential. Remarkably, this helicoid potential can be simply realized in minimal supergravity. The global U(1)U(1) symmetry of the K\"ahler potential introduces a flat direction and evades the η\eta problem automatically. So such inflation is technically natural. The phase excursion is super-Planckian as required by the Lyth bound, while the norm of the complex field can be suppressed in the sub-Planckian region. This model resolves the ultraviolet sensitive problem of the large field inflation, besides, it also provides a new type of monodromy inflation in supersymmetric field theory with consistent field stabilization.

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