On supersymmetry breaking vacua from D-branes at orientifold singularities
Abstract We present a large class of models of D-branes at (orientifold) Calabi-Yau sin- gularities which enjoy dynamical supersymmetry breaking at low energy, by means of either the SU(5) or 3–2 supersymmetry breaking models. Once embedded in a warped throat or, equivalently, in a large N theory, a...
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Online Access: | https://doi.org/10.1007/JHEP12(2019)145 |
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doaj-dbc25135c8a541acb62edcf6b8c4873d2020-12-20T12:05:14ZengSpringerOpenJournal of High Energy Physics1029-84792019-12-0120191214610.1007/JHEP12(2019)145On supersymmetry breaking vacua from D-branes at orientifold singularitiesRiccardo Argurio0Matteo Bertolini1Shani Meynet2Antoine Pasternak3Physique Théorique et Mathématique and International Solvay Institutes, Université Libre de BruxellesSISSA and INFNICTPPhysique Théorique et Mathématique and International Solvay Institutes, Université Libre de BruxellesAbstract We present a large class of models of D-branes at (orientifold) Calabi-Yau sin- gularities which enjoy dynamical supersymmetry breaking at low energy, by means of either the SU(5) or 3–2 supersymmetry breaking models. Once embedded in a warped throat or, equivalently, in a large N theory, all models display an instability along a Coulomb branch direction towards supersymmetry preserving vacua. Interestingly, the nature of the run- away mechanism is model-independent and has a precise geometrical interpretation. This naturally suggests the properties a Calabi-Yau singularity should have in order for such instability not to occur.https://doi.org/10.1007/JHEP12(2019)145D-branesGauge-gravity correspondenceSupersymmetric Gauge TheorySupersymmetry Breaking |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Riccardo Argurio Matteo Bertolini Shani Meynet Antoine Pasternak |
spellingShingle |
Riccardo Argurio Matteo Bertolini Shani Meynet Antoine Pasternak On supersymmetry breaking vacua from D-branes at orientifold singularities Journal of High Energy Physics D-branes Gauge-gravity correspondence Supersymmetric Gauge Theory Supersymmetry Breaking |
author_facet |
Riccardo Argurio Matteo Bertolini Shani Meynet Antoine Pasternak |
author_sort |
Riccardo Argurio |
title |
On supersymmetry breaking vacua from D-branes at orientifold singularities |
title_short |
On supersymmetry breaking vacua from D-branes at orientifold singularities |
title_full |
On supersymmetry breaking vacua from D-branes at orientifold singularities |
title_fullStr |
On supersymmetry breaking vacua from D-branes at orientifold singularities |
title_full_unstemmed |
On supersymmetry breaking vacua from D-branes at orientifold singularities |
title_sort |
on supersymmetry breaking vacua from d-branes at orientifold singularities |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2019-12-01 |
description |
Abstract We present a large class of models of D-branes at (orientifold) Calabi-Yau sin- gularities which enjoy dynamical supersymmetry breaking at low energy, by means of either the SU(5) or 3–2 supersymmetry breaking models. Once embedded in a warped throat or, equivalently, in a large N theory, all models display an instability along a Coulomb branch direction towards supersymmetry preserving vacua. Interestingly, the nature of the run- away mechanism is model-independent and has a precise geometrical interpretation. This naturally suggests the properties a Calabi-Yau singularity should have in order for such instability not to occur. |
topic |
D-branes Gauge-gravity correspondence Supersymmetric Gauge Theory Supersymmetry Breaking |
url |
https://doi.org/10.1007/JHEP12(2019)145 |
work_keys_str_mv |
AT riccardoargurio onsupersymmetrybreakingvacuafromdbranesatorientifoldsingularities AT matteobertolini onsupersymmetrybreakingvacuafromdbranesatorientifoldsingularities AT shanimeynet onsupersymmetrybreakingvacuafromdbranesatorientifoldsingularities AT antoinepasternak onsupersymmetrybreakingvacuafromdbranesatorientifoldsingularities |
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1724377125077647360 |