UV corrections in sgoldstino-less inflation

We study the embedding of inflation with nilpotent multiplets in supergravity, in particular the decoupling of the sgoldstino scalar field. Instead of being imposed by hand, the nilpotency constraint on the goldstino multiplet arises in the low energy-effective theory by integrating out heavy degree...

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Main Authors: Emilian Dudas, Lucien Heurtier, Clemens Wieck, Martin Wolfgang Winkler
Format: Article
Language:English
Published: Elsevier 2016-08-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316302192
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spelling doaj-9a53523921394c0f9efd4808a4dda8e42020-11-24T22:43:21ZengElsevierPhysics Letters B0370-26931873-24452016-08-01759C12112510.1016/j.physletb.2016.05.072UV corrections in sgoldstino-less inflationEmilian Dudas0Lucien Heurtier1Clemens Wieck2Martin Wolfgang Winkler3Centre de Physique Théorique, Ecole Polytechnique, CNRS, Univ. Paris-Saclay, 91128 Palaiseau Cedex, FranceService de Physique Théorique, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, 1050 Brussels, BelgiumDepartamento de Física Teórica UAM and Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid Cantoblanco, 28049 Madrid, SpainBethe Center for Theoretical Physics and Physikalisches Institut der Universität Bonn, Nussallee 12, 53115 Bonn, GermanyWe study the embedding of inflation with nilpotent multiplets in supergravity, in particular the decoupling of the sgoldstino scalar field. Instead of being imposed by hand, the nilpotency constraint on the goldstino multiplet arises in the low energy-effective theory by integrating out heavy degrees of freedom. We present explicit supergravity models in which a large but finite sgoldstino mass arises from Yukawa or gauge interactions. In both cases the inflaton potential receives two types of corrections. One is from the backreaction of the sgoldstino, the other from the heavy fields generating its mass. We show that these scale oppositely with the Volkov–Akulov cut-off scale, which makes a consistent decoupling of the sgoldstino nontrivial. Still, we identify a parameter window in which sgoldstino-less inflation can take place, up to corrections which flatten the inflaton potential.http://www.sciencedirect.com/science/article/pii/S0370269316302192
collection DOAJ
language English
format Article
sources DOAJ
author Emilian Dudas
Lucien Heurtier
Clemens Wieck
Martin Wolfgang Winkler
spellingShingle Emilian Dudas
Lucien Heurtier
Clemens Wieck
Martin Wolfgang Winkler
UV corrections in sgoldstino-less inflation
Physics Letters B
author_facet Emilian Dudas
Lucien Heurtier
Clemens Wieck
Martin Wolfgang Winkler
author_sort Emilian Dudas
title UV corrections in sgoldstino-less inflation
title_short UV corrections in sgoldstino-less inflation
title_full UV corrections in sgoldstino-less inflation
title_fullStr UV corrections in sgoldstino-less inflation
title_full_unstemmed UV corrections in sgoldstino-less inflation
title_sort uv corrections in sgoldstino-less inflation
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2016-08-01
description We study the embedding of inflation with nilpotent multiplets in supergravity, in particular the decoupling of the sgoldstino scalar field. Instead of being imposed by hand, the nilpotency constraint on the goldstino multiplet arises in the low energy-effective theory by integrating out heavy degrees of freedom. We present explicit supergravity models in which a large but finite sgoldstino mass arises from Yukawa or gauge interactions. In both cases the inflaton potential receives two types of corrections. One is from the backreaction of the sgoldstino, the other from the heavy fields generating its mass. We show that these scale oppositely with the Volkov–Akulov cut-off scale, which makes a consistent decoupling of the sgoldstino nontrivial. Still, we identify a parameter window in which sgoldstino-less inflation can take place, up to corrections which flatten the inflaton potential.
url http://www.sciencedirect.com/science/article/pii/S0370269316302192
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AT lucienheurtier uvcorrectionsinsgoldstinolessinflation
AT clemenswieck uvcorrectionsinsgoldstinolessinflation
AT martinwolfgangwinkler uvcorrectionsinsgoldstinolessinflation
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