Axion inflation in F-theory

We study the dynamics of axion-like fields in F-theory and suggest that they can serve as inflatons in models of natural inflation. The axions arise from harmonic three-forms on the F-theory compactification space and parameterize a complex torus that varies over the geometric moduli space. In parti...

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Main Author: Thomas W. Grimm
Format: Article
Language:English
Published: Elsevier 2014-12-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269314007667
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author Thomas W. Grimm
author_facet Thomas W. Grimm
author_sort Thomas W. Grimm
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description We study the dynamics of axion-like fields in F-theory and suggest that they can serve as inflatons in models of natural inflation. The axions arise from harmonic three-forms on the F-theory compactification space and parameterize a complex torus that varies over the geometric moduli space. In particular, this implies that the axion decay constants depend on the complex structure moduli that can be fixed by background fluxes. This might allow tuning them to be super-Planckian in a controlled way and allow for interesting single field inflationary models. We argue that this requires a localization of the three-forms near regions of strong string coupling, analogously to the reasoning that GUT physics requires the use of F-theory. These models can admit a tensor to scalar ratio r>0.1.
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spelling doaj.art-e0756010016e4583a807d6ef9382a48f2022-12-22T03:32:19ZengElsevierPhysics Letters B0370-26932014-12-01739201208Axion inflation in F-theoryThomas W. Grimm0Max-Planck-Institut für Physik, Föhringer Ring 6, 80805 Munich, GermanyWe study the dynamics of axion-like fields in F-theory and suggest that they can serve as inflatons in models of natural inflation. The axions arise from harmonic three-forms on the F-theory compactification space and parameterize a complex torus that varies over the geometric moduli space. In particular, this implies that the axion decay constants depend on the complex structure moduli that can be fixed by background fluxes. This might allow tuning them to be super-Planckian in a controlled way and allow for interesting single field inflationary models. We argue that this requires a localization of the three-forms near regions of strong string coupling, analogously to the reasoning that GUT physics requires the use of F-theory. These models can admit a tensor to scalar ratio r>0.1.http://www.sciencedirect.com/science/article/pii/S0370269314007667
spellingShingle Thomas W. Grimm
Axion inflation in F-theory
Physics Letters B
title Axion inflation in F-theory
title_full Axion inflation in F-theory
title_fullStr Axion inflation in F-theory
title_full_unstemmed Axion inflation in F-theory
title_short Axion inflation in F-theory
title_sort axion inflation in f theory
url http://www.sciencedirect.com/science/article/pii/S0370269314007667
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