Unified model of chaotic inflation and dynamical supersymmetry breaking

The large hierarchy between the Planck scale and the weak scale can be explained by the dynamical breaking of supersymmetry in strongly coupled gauge theories. Similarly, the hierarchy between the Planck scale and the energy scale of inflation may also originate from strong dynamics, which dynamical...

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Main Authors: Keisuke Harigaya, Kai Schmitz
Format: Article
Language:English
Published: Elsevier 2017-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S037026931730672X
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spelling doaj-ff858dfe67ba4efaab58fec16a6c3b0d2020-11-24T21:43:01ZengElsevierPhysics Letters B0370-26932017-10-01773320324Unified model of chaotic inflation and dynamical supersymmetry breakingKeisuke Harigaya0Kai Schmitz1Department of Physics, University of California, Berkeley, CA 94720, USA; Theoretical Physics Group, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA; Corresponding authors.Max-Planck-Institut für Kernphysik (MPIK), 69117 Heidelberg, Germany; Corresponding authors.The large hierarchy between the Planck scale and the weak scale can be explained by the dynamical breaking of supersymmetry in strongly coupled gauge theories. Similarly, the hierarchy between the Planck scale and the energy scale of inflation may also originate from strong dynamics, which dynamically generate the inflaton potential. We present a model of the hidden sector which unifies these two ideas, i.e., in which the scales of inflation and supersymmetry breaking are provided by the dynamics of the same gauge group. The resultant inflation model is chaotic inflation with a fractional power-law potential in accord with the upper bound on the tensor-to-scalar ratio. The supersymmetry breaking scale can be much smaller than the inflation scale, so that the solution to the large hierarchy problem of the weak scale remains intact. As an intrinsic feature of our model, we find that the sgoldstino, which might disturb the inflationary dynamics, is automatically stabilized during inflation by dynamically generated corrections in the strongly coupled sector. This renders our model a field-theoretical realization of what is sometimes referred to as sgoldstino-less inflation.http://www.sciencedirect.com/science/article/pii/S037026931730672X
collection DOAJ
language English
format Article
sources DOAJ
author Keisuke Harigaya
Kai Schmitz
spellingShingle Keisuke Harigaya
Kai Schmitz
Unified model of chaotic inflation and dynamical supersymmetry breaking
Physics Letters B
author_facet Keisuke Harigaya
Kai Schmitz
author_sort Keisuke Harigaya
title Unified model of chaotic inflation and dynamical supersymmetry breaking
title_short Unified model of chaotic inflation and dynamical supersymmetry breaking
title_full Unified model of chaotic inflation and dynamical supersymmetry breaking
title_fullStr Unified model of chaotic inflation and dynamical supersymmetry breaking
title_full_unstemmed Unified model of chaotic inflation and dynamical supersymmetry breaking
title_sort unified model of chaotic inflation and dynamical supersymmetry breaking
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2017-10-01
description The large hierarchy between the Planck scale and the weak scale can be explained by the dynamical breaking of supersymmetry in strongly coupled gauge theories. Similarly, the hierarchy between the Planck scale and the energy scale of inflation may also originate from strong dynamics, which dynamically generate the inflaton potential. We present a model of the hidden sector which unifies these two ideas, i.e., in which the scales of inflation and supersymmetry breaking are provided by the dynamics of the same gauge group. The resultant inflation model is chaotic inflation with a fractional power-law potential in accord with the upper bound on the tensor-to-scalar ratio. The supersymmetry breaking scale can be much smaller than the inflation scale, so that the solution to the large hierarchy problem of the weak scale remains intact. As an intrinsic feature of our model, we find that the sgoldstino, which might disturb the inflationary dynamics, is automatically stabilized during inflation by dynamically generated corrections in the strongly coupled sector. This renders our model a field-theoretical realization of what is sometimes referred to as sgoldstino-less inflation.
url http://www.sciencedirect.com/science/article/pii/S037026931730672X
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