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...
Main Authors: | , |
---|---|
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 |