Symmetry breaking patterns for inflation

Abstract We study inflationary models where the kinetic sector of the theory has a non-linearly realised symmetry which is broken by the inflationary potential. We distinguish between kinetic symmetries which non-linearly realise an internal or space-time group, and which yield a flat or curved scal...

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Main Authors: Remko Klein, Diederik Roest, David Stefanyszyn
Format: Article
Language:English
Published: SpringerOpen 2018-06-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP06(2018)006
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spelling doaj-c0059c0721cf4569b6053df2be6f7f892020-11-25T01:02:29ZengSpringerOpenJournal of High Energy Physics1029-84792018-06-012018612310.1007/JHEP06(2018)006Symmetry breaking patterns for inflationRemko Klein0Diederik Roest1David Stefanyszyn2Van Swinderen Institute for Particle Physics and Gravity, University of GroningenVan Swinderen Institute for Particle Physics and Gravity, University of GroningenVan Swinderen Institute for Particle Physics and Gravity, University of GroningenAbstract We study inflationary models where the kinetic sector of the theory has a non-linearly realised symmetry which is broken by the inflationary potential. We distinguish between kinetic symmetries which non-linearly realise an internal or space-time group, and which yield a flat or curved scalar manifold. This classification leads to well-known inflationary models such as monomial inflation and α-attractors, as well as a new model based on fixed couplings between a dilaton and many axions which non-linearly realises higher-dimensional conformal symmetries. In this model, inflation can be realised along the dilatonic direction, leading to a tensor-to-scalar ratio r ∼ 0.01 and a spectral index n s ∼ 0.975. We refer to the new model as ambient inflation since inflation proceeds along an isometry of an anti-de Sitter ambient space-time, which fully determines the kinetic sector.http://link.springer.com/article/10.1007/JHEP06(2018)006Effective Field TheoriesGlobal SymmetriesSpace-Time Symmetries
collection DOAJ
language English
format Article
sources DOAJ
author Remko Klein
Diederik Roest
David Stefanyszyn
spellingShingle Remko Klein
Diederik Roest
David Stefanyszyn
Symmetry breaking patterns for inflation
Journal of High Energy Physics
Effective Field Theories
Global Symmetries
Space-Time Symmetries
author_facet Remko Klein
Diederik Roest
David Stefanyszyn
author_sort Remko Klein
title Symmetry breaking patterns for inflation
title_short Symmetry breaking patterns for inflation
title_full Symmetry breaking patterns for inflation
title_fullStr Symmetry breaking patterns for inflation
title_full_unstemmed Symmetry breaking patterns for inflation
title_sort symmetry breaking patterns for inflation
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-06-01
description Abstract We study inflationary models where the kinetic sector of the theory has a non-linearly realised symmetry which is broken by the inflationary potential. We distinguish between kinetic symmetries which non-linearly realise an internal or space-time group, and which yield a flat or curved scalar manifold. This classification leads to well-known inflationary models such as monomial inflation and α-attractors, as well as a new model based on fixed couplings between a dilaton and many axions which non-linearly realises higher-dimensional conformal symmetries. In this model, inflation can be realised along the dilatonic direction, leading to a tensor-to-scalar ratio r ∼ 0.01 and a spectral index n s ∼ 0.975. We refer to the new model as ambient inflation since inflation proceeds along an isometry of an anti-de Sitter ambient space-time, which fully determines the kinetic sector.
topic Effective Field Theories
Global Symmetries
Space-Time Symmetries
url http://link.springer.com/article/10.1007/JHEP06(2018)006
work_keys_str_mv AT remkoklein symmetrybreakingpatternsforinflation
AT diederikroest symmetrybreakingpatternsforinflation
AT davidstefanyszyn symmetrybreakingpatternsforinflation
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