Three-form multiplet and supersymmetry breaking

Abstract Recently, a nilpotent real scalar superfield V was introduced in [1] as a model for the Goldstino. It contains only two independent component fields, the Goldstino and the auxiliary D-field. Here we first show that V can equivalently be realised as a constrained three-form superfield. We de...

Full description

Bibliographic Details
Main Authors: Evgeny I. Buchbinder, Sergei M. Kuzenko
Format: Article
Language:English
Published: SpringerOpen 2017-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP09(2017)089
id doaj-4ab837fd317449d1b24bb4874e561b5b
record_format Article
spelling doaj-4ab837fd317449d1b24bb4874e561b5b2020-11-24T21:38:51ZengSpringerOpenJournal of High Energy Physics1029-84792017-09-012017911710.1007/JHEP09(2017)089Three-form multiplet and supersymmetry breakingEvgeny I. Buchbinder0Sergei M. Kuzenko1School of Physics and Astrophysics M013, The University of Western AustraliaSchool of Physics and Astrophysics M013, The University of Western AustraliaAbstract Recently, a nilpotent real scalar superfield V was introduced in [1] as a model for the Goldstino. It contains only two independent component fields, the Goldstino and the auxiliary D-field. Here we first show that V can equivalently be realised as a constrained three-form superfield. We demonstrate that every irreducible Goldstino superfield (of which the Goldstino is the only independent component field) can be realised as a descendant of V which is invariant under local rescalings V → e τ V, where τ is an arbitrary real scalar superfield. We next propose a new Goldstino supermultiplet which is described by a nilpotent three-form superfield Y $$ \mathcal{Y} $$ that is a variant formulation for the nilpotent chiral superfield, which is often used in off-shell models for spontaneously broken supergravity. It is shown that the action describing the dynamics of Y $$ \mathcal{Y} $$ may be obtained from a super-symmetric nonlinear σ-model in the infrared limit. Unlike V , the Goldstino superfield Y $$ \mathcal{Y} $$ contains two independent auxiliary fields, F = H + iG, of which H is a scalar and G is the field strength of a gauge three-form. When Y $$ \mathcal{Y} $$ is coupled to supergravity, both H and G produce positive contributions to the cosmological constant. While the contribution from H is uniquely determined by the parameter of the supersymmetry breaking in the action, the contribution from G is dynamical.http://link.springer.com/article/10.1007/JHEP09(2017)089SuperspacesSupersymmetry Breaking
collection DOAJ
language English
format Article
sources DOAJ
author Evgeny I. Buchbinder
Sergei M. Kuzenko
spellingShingle Evgeny I. Buchbinder
Sergei M. Kuzenko
Three-form multiplet and supersymmetry breaking
Journal of High Energy Physics
Superspaces
Supersymmetry Breaking
author_facet Evgeny I. Buchbinder
Sergei M. Kuzenko
author_sort Evgeny I. Buchbinder
title Three-form multiplet and supersymmetry breaking
title_short Three-form multiplet and supersymmetry breaking
title_full Three-form multiplet and supersymmetry breaking
title_fullStr Three-form multiplet and supersymmetry breaking
title_full_unstemmed Three-form multiplet and supersymmetry breaking
title_sort three-form multiplet and supersymmetry breaking
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2017-09-01
description Abstract Recently, a nilpotent real scalar superfield V was introduced in [1] as a model for the Goldstino. It contains only two independent component fields, the Goldstino and the auxiliary D-field. Here we first show that V can equivalently be realised as a constrained three-form superfield. We demonstrate that every irreducible Goldstino superfield (of which the Goldstino is the only independent component field) can be realised as a descendant of V which is invariant under local rescalings V → e τ V, where τ is an arbitrary real scalar superfield. We next propose a new Goldstino supermultiplet which is described by a nilpotent three-form superfield Y $$ \mathcal{Y} $$ that is a variant formulation for the nilpotent chiral superfield, which is often used in off-shell models for spontaneously broken supergravity. It is shown that the action describing the dynamics of Y $$ \mathcal{Y} $$ may be obtained from a super-symmetric nonlinear σ-model in the infrared limit. Unlike V , the Goldstino superfield Y $$ \mathcal{Y} $$ contains two independent auxiliary fields, F = H + iG, of which H is a scalar and G is the field strength of a gauge three-form. When Y $$ \mathcal{Y} $$ is coupled to supergravity, both H and G produce positive contributions to the cosmological constant. While the contribution from H is uniquely determined by the parameter of the supersymmetry breaking in the action, the contribution from G is dynamical.
topic Superspaces
Supersymmetry Breaking
url http://link.springer.com/article/10.1007/JHEP09(2017)089
work_keys_str_mv AT evgenyibuchbinder threeformmultipletandsupersymmetrybreaking
AT sergeimkuzenko threeformmultipletandsupersymmetrybreaking
_version_ 1725934166598483968