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Helical Phase Inflation

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arxiv 1409.3267 v2 pith:SPY5DM6R submitted 2014-09-10 hep-th astro-ph.COhep-ph

classification hep-thastro-ph.COhep-ph
keywords fieldinflationphasepotentialcomplexhelicoidproblemrealized
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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 $U(1)$ symmetry of the K\"ahler potential introduces a flat direction and evades the $\eta$ 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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  1. Helical phase inflation and its observational constraints

    hep-ph 2019-08 conditional novelty 5.0 of 10

    Helical phase inflation, using the phase of a complex scalar as the inflaton, fits Planck 2018 and BICEP2 data and is claimed to show alpha-attractor behavior, with a brane version that reduces field excursions.

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