Fayet–Iliopoulos terms in supergravity and D-term inflation

Abstract We analyse the consequences of a new gauge invariant Fayet–Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that charged matter fields can be consistently added wit...

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Main Authors: I. Antoniadis, A. Chatrabhuti, H. Isono, R. Knoops
Format: Article
Language:English
Published: SpringerOpen 2018-05-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-5861-6
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spelling doaj-cee8cd1b2054422c8e5caee9fed023f62020-11-24T22:23:21ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-05-0178511110.1140/epjc/s10052-018-5861-6Fayet–Iliopoulos terms in supergravity and D-term inflationI. Antoniadis0A. Chatrabhuti1H. Isono2R. Knoops3Laboratoire de Physique Théorique et Hautes Energies - LPTHE, Sorbonne Université, CNRSDepartment of Physics, Faculty of Science, Chulalongkorn UniversityDepartment of Physics, Faculty of Science, Chulalongkorn UniversityDepartment of Physics, Faculty of Science, Chulalongkorn UniversityAbstract We analyse the consequences of a new gauge invariant Fayet–Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that charged matter fields can be consistently added with the new term, as well as the standard FI term in supergravity in a Kähler frame where the U(1) is not an R-symmetry. We then show that the slow-roll conditions can be easily satisfied with inflation driven by a D-term depending on the two FI parameters. Inflation starts at initial conditions around the maximum of the potential where the U(1) symmetry is restored and stops when the inflaton rolls down to the minimum describing the present phase of our Universe. The resulting tensor-to-scalar ratio of primordial perturbations can be even at observable values in the presence of higher order terms in the Kähler potential.http://link.springer.com/article/10.1140/epjc/s10052-018-5861-6
collection DOAJ
language English
format Article
sources DOAJ
author I. Antoniadis
A. Chatrabhuti
H. Isono
R. Knoops
spellingShingle I. Antoniadis
A. Chatrabhuti
H. Isono
R. Knoops
Fayet–Iliopoulos terms in supergravity and D-term inflation
European Physical Journal C: Particles and Fields
author_facet I. Antoniadis
A. Chatrabhuti
H. Isono
R. Knoops
author_sort I. Antoniadis
title Fayet–Iliopoulos terms in supergravity and D-term inflation
title_short Fayet–Iliopoulos terms in supergravity and D-term inflation
title_full Fayet–Iliopoulos terms in supergravity and D-term inflation
title_fullStr Fayet–Iliopoulos terms in supergravity and D-term inflation
title_full_unstemmed Fayet–Iliopoulos terms in supergravity and D-term inflation
title_sort fayet–iliopoulos terms in supergravity and d-term inflation
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2018-05-01
description Abstract We analyse the consequences of a new gauge invariant Fayet–Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that charged matter fields can be consistently added with the new term, as well as the standard FI term in supergravity in a Kähler frame where the U(1) is not an R-symmetry. We then show that the slow-roll conditions can be easily satisfied with inflation driven by a D-term depending on the two FI parameters. Inflation starts at initial conditions around the maximum of the potential where the U(1) symmetry is restored and stops when the inflaton rolls down to the minimum describing the present phase of our Universe. The resulting tensor-to-scalar ratio of primordial perturbations can be even at observable values in the presence of higher order terms in the Kähler potential.
url http://link.springer.com/article/10.1140/epjc/s10052-018-5861-6
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