Next-to-minimal dark matter at the LHC
Abstract We examine the collider signatures of a WIMP dark matter scenario comprising a singlet fermion and an SU(2) n-plet fermion, with a focus on n = 3 and n = 5. The singlet and n-plet masses are of the order of the electroweak scale. The n-plet contains new charged particles which will be copio...
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Online Access: | http://link.springer.com/article/10.1007/JHEP11(2018)195 |
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doaj-199919f373254c2d80e2660a12786d9f2020-11-25T00:57:42ZengSpringerOpenJournal of High Energy Physics1029-84792018-11-0120181112010.1007/JHEP11(2018)195Next-to-minimal dark matter at the LHCA. Bharucha0F. Brümmer1N. Desai2Aix Marseille Univ, Université de Toulon, CNRS, CPT, Marseille, FranceLUPM, UMR5299, Université de Montpellier and CNRSLUPM, UMR5299, Université de Montpellier and CNRSAbstract We examine the collider signatures of a WIMP dark matter scenario comprising a singlet fermion and an SU(2) n-plet fermion, with a focus on n = 3 and n = 5. The singlet and n-plet masses are of the order of the electroweak scale. The n-plet contains new charged particles which will be copiously pair-produced at the LHC. Small mixing angles and near-degenerate masses, both of which feature naturally in these models, give rise to long-lived particles and their characteristic collider signatures. In particular, the n = 5 model can be constrained by displaced lepton searches independently of the mixing angle, generically ruling out 5-plet masses below about 280 GeV. For small mixing angles, we show that there is a parameter range for which the model reproduces the observed thermal relic density but is severely constrained by disappearing track searches in both the n = 3 and the n = 5 cases. The n = 3 model is further constrained by soft di-lepton searches irrespective of whether any of the new particles are long-lived.http://link.springer.com/article/10.1007/JHEP11(2018)195Beyond Standard ModelEffective Field Theories |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
A. Bharucha F. Brümmer N. Desai |
spellingShingle |
A. Bharucha F. Brümmer N. Desai Next-to-minimal dark matter at the LHC Journal of High Energy Physics Beyond Standard Model Effective Field Theories |
author_facet |
A. Bharucha F. Brümmer N. Desai |
author_sort |
A. Bharucha |
title |
Next-to-minimal dark matter at the LHC |
title_short |
Next-to-minimal dark matter at the LHC |
title_full |
Next-to-minimal dark matter at the LHC |
title_fullStr |
Next-to-minimal dark matter at the LHC |
title_full_unstemmed |
Next-to-minimal dark matter at the LHC |
title_sort |
next-to-minimal dark matter at the lhc |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2018-11-01 |
description |
Abstract We examine the collider signatures of a WIMP dark matter scenario comprising a singlet fermion and an SU(2) n-plet fermion, with a focus on n = 3 and n = 5. The singlet and n-plet masses are of the order of the electroweak scale. The n-plet contains new charged particles which will be copiously pair-produced at the LHC. Small mixing angles and near-degenerate masses, both of which feature naturally in these models, give rise to long-lived particles and their characteristic collider signatures. In particular, the n = 5 model can be constrained by displaced lepton searches independently of the mixing angle, generically ruling out 5-plet masses below about 280 GeV. For small mixing angles, we show that there is a parameter range for which the model reproduces the observed thermal relic density but is severely constrained by disappearing track searches in both the n = 3 and the n = 5 cases. The n = 3 model is further constrained by soft di-lepton searches irrespective of whether any of the new particles are long-lived. |
topic |
Beyond Standard Model Effective Field Theories |
url |
http://link.springer.com/article/10.1007/JHEP11(2018)195 |
work_keys_str_mv |
AT abharucha nexttominimaldarkmatteratthelhc AT fbrummer nexttominimaldarkmatteratthelhc AT ndesai nexttominimaldarkmatteratthelhc |
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1725222702153728000 |