Salvage of too slow gravitinos
Abstract Gravitinos can inherit a non-relativistic dispersion relation while propagating in a background breaking both supersymmetry and Lorentz symmetry spontaneously. This is because the longitudinal mode velocity is controlled by the sound speed in the background. It was pointed out recently by K...
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2021
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oai:doaj.org-article:0482feeccc6e45ea9d0dfa6681cf8d5f2021-11-14T12:40:43ZSalvage of too slow gravitinos10.1007/JHEP11(2021)0631029-8479https://doaj.org/article/0482feeccc6e45ea9d0dfa6681cf8d5f2021-11-01T00:00:00Zhttps://doi.org/10.1007/JHEP11(2021)063https://doaj.org/toc/1029-8479Abstract Gravitinos can inherit a non-relativistic dispersion relation while propagating in a background breaking both supersymmetry and Lorentz symmetry spontaneously. This is because the longitudinal mode velocity is controlled by the sound speed in the background. It was pointed out recently by Kolb, Long and McDonough that the production of gravitinos might diverge when this sound speed vanishes. We argue that in the framework of cosmological models with linearly spontaneously broken realised supersymmetry, where the physical fermions are combinations of the vacuum goldstino and the inflatino, the gravitino longitudinal mode has a relativistic dispersion relation and therefore avoids the catastrophic production. We illustrate this in some explicit examples.I. AntoniadisK. BenakliW. KeSpringerOpenarticleBeyond Standard ModelCosmology of Theories beyond the SMSupergravity ModelsNuclear and particle physics. Atomic energy. RadioactivityQC770-798ENJournal of High Energy Physics, Vol 2021, Iss 11, Pp 1-16 (2021) |
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Beyond Standard Model Cosmology of Theories beyond the SM Supergravity Models Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Beyond Standard Model Cosmology of Theories beyond the SM Supergravity Models Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 I. Antoniadis K. Benakli W. Ke Salvage of too slow gravitinos |
description |
Abstract Gravitinos can inherit a non-relativistic dispersion relation while propagating in a background breaking both supersymmetry and Lorentz symmetry spontaneously. This is because the longitudinal mode velocity is controlled by the sound speed in the background. It was pointed out recently by Kolb, Long and McDonough that the production of gravitinos might diverge when this sound speed vanishes. We argue that in the framework of cosmological models with linearly spontaneously broken realised supersymmetry, where the physical fermions are combinations of the vacuum goldstino and the inflatino, the gravitino longitudinal mode has a relativistic dispersion relation and therefore avoids the catastrophic production. We illustrate this in some explicit examples. |
format |
article |
author |
I. Antoniadis K. Benakli W. Ke |
author_facet |
I. Antoniadis K. Benakli W. Ke |
author_sort |
I. Antoniadis |
title |
Salvage of too slow gravitinos |
title_short |
Salvage of too slow gravitinos |
title_full |
Salvage of too slow gravitinos |
title_fullStr |
Salvage of too slow gravitinos |
title_full_unstemmed |
Salvage of too slow gravitinos |
title_sort |
salvage of too slow gravitinos |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/0482feeccc6e45ea9d0dfa6681cf8d5f |
work_keys_str_mv |
AT iantoniadis salvageoftooslowgravitinos AT kbenakli salvageoftooslowgravitinos AT wke salvageoftooslowgravitinos |
_version_ |
1718429086857035776 |