Harmonic hybrid inflation

Abstract We present a mechanism for realizing hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. The structure of the scalar potential is highly constrained by the discrete shift symmetries of the axions. We show that harmonic hybrid inflation genera...

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Main Authors: Federico Carta, Nicole Righi, Yvette Welling, Alexander Westphal
Format: Article
Language:English
Published: SpringerOpen 2020-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2020)161
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spelling doaj-282d9c4157a740b7ba923c9647094b682020-12-27T12:02:57ZengSpringerOpenJournal of High Energy Physics1029-84792020-12-0120201213210.1007/JHEP12(2020)161Harmonic hybrid inflationFederico Carta0Nicole Righi1Yvette Welling2Alexander Westphal3Deutsches Elektronen-Synchrotron DESY, Theory GroupDeutsches Elektronen-Synchrotron DESY, Theory GroupDeutsches Elektronen-Synchrotron DESY, Theory GroupDeutsches Elektronen-Synchrotron DESY, Theory GroupAbstract We present a mechanism for realizing hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. The structure of the scalar potential is highly constrained by the discrete shift symmetries of the axions. We show that harmonic hybrid inflation generates observationally viable slow-roll inflation for a wide range of initial conditions. This is possible while accommodating certain UV arguments favoring constraints f ≲ M P and ∆ϕ 60 ≲ M P on the axion periodicity and slow-roll field range, respectively. We discuss controlled ℤ2-symmetry breaking of the adjacent axion vacua as a means of avoiding cosmological domain wall problems. Including a minimal form of ℤ2-symmetry breaking into the minimally tuned setup leads to a prediction of primordial tensor modes with the tensor-to-scalar ratio in the range 10 −4 ≲ r ≲ 0.01, directly accessible to upcoming CMB observations. Finally, we outline several avenues towards realizing harmonic hybrid inflation in type IIB string theory.https://doi.org/10.1007/JHEP12(2020)161Strings and branes phenomenology
collection DOAJ
language English
format Article
sources DOAJ
author Federico Carta
Nicole Righi
Yvette Welling
Alexander Westphal
spellingShingle Federico Carta
Nicole Righi
Yvette Welling
Alexander Westphal
Harmonic hybrid inflation
Journal of High Energy Physics
Strings and branes phenomenology
author_facet Federico Carta
Nicole Righi
Yvette Welling
Alexander Westphal
author_sort Federico Carta
title Harmonic hybrid inflation
title_short Harmonic hybrid inflation
title_full Harmonic hybrid inflation
title_fullStr Harmonic hybrid inflation
title_full_unstemmed Harmonic hybrid inflation
title_sort harmonic hybrid inflation
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-12-01
description Abstract We present a mechanism for realizing hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. The structure of the scalar potential is highly constrained by the discrete shift symmetries of the axions. We show that harmonic hybrid inflation generates observationally viable slow-roll inflation for a wide range of initial conditions. This is possible while accommodating certain UV arguments favoring constraints f ≲ M P and ∆ϕ 60 ≲ M P on the axion periodicity and slow-roll field range, respectively. We discuss controlled ℤ2-symmetry breaking of the adjacent axion vacua as a means of avoiding cosmological domain wall problems. Including a minimal form of ℤ2-symmetry breaking into the minimally tuned setup leads to a prediction of primordial tensor modes with the tensor-to-scalar ratio in the range 10 −4 ≲ r ≲ 0.01, directly accessible to upcoming CMB observations. Finally, we outline several avenues towards realizing harmonic hybrid inflation in type IIB string theory.
topic Strings and branes phenomenology
url https://doi.org/10.1007/JHEP12(2020)161
work_keys_str_mv AT federicocarta harmonichybridinflation
AT nicolerighi harmonichybridinflation
AT yvettewelling harmonichybridinflation
AT alexanderwestphal harmonichybridinflation
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