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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2016-08-01
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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 |
work_keys_str_mv |
AT emiliandudas uvcorrectionsinsgoldstinolessinflation AT lucienheurtier uvcorrectionsinsgoldstinolessinflation AT clemenswieck uvcorrectionsinsgoldstinolessinflation AT martinwolfgangwinkler uvcorrectionsinsgoldstinolessinflation |
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