Well-tempered n-plet dark matter
Abstract We study simple effective models of fermionic WIMP dark matter, where the dark matter candidate is a mixture of a Standard Model singlet and an n-plet of SU2 L with n ≥ 3, stabilized by a discrete symmetry. The dark matter mass is assumed to be around the electroweak scale, and the mixing i...
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Online Access: | http://link.springer.com/article/10.1007/JHEP09(2017)160 |
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doaj-7943cb467a4e4a0c882c81ed5d8ad4582020-11-25T01:26:48ZengSpringerOpenJournal of High Energy Physics1029-84792017-09-012017912810.1007/JHEP09(2017)160Well-tempered n-plet dark matterA. Bharucha0F. Brümmer1R. Ruffault2CPT, UMR7332, CNRS and Aix-Marseille Université and Université de ToulonLUPM, UMR5299, Université de Montpellier and CNRSLUPM, UMR5299, Université de Montpellier and CNRSAbstract We study simple effective models of fermionic WIMP dark matter, where the dark matter candidate is a mixture of a Standard Model singlet and an n-plet of SU2 L with n ≥ 3, stabilized by a discrete symmetry. The dark matter mass is assumed to be around the electroweak scale, and the mixing is generated by higher-dimensional operators, with a cutoff scale ≳TeV. For appropriate values of the mass parameters and the mixing we find that the observed dark matter relic density can be generated by coannihilation. Direct detection experiments have already excluded large parts of the parameter space, and the next-generation experiments will further constrain these models.http://link.springer.com/article/10.1007/JHEP09(2017)160Beyond Standard ModelCosmology of Theories beyond the SM |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
A. Bharucha F. Brümmer R. Ruffault |
spellingShingle |
A. Bharucha F. Brümmer R. Ruffault Well-tempered n-plet dark matter Journal of High Energy Physics Beyond Standard Model Cosmology of Theories beyond the SM |
author_facet |
A. Bharucha F. Brümmer R. Ruffault |
author_sort |
A. Bharucha |
title |
Well-tempered n-plet dark matter |
title_short |
Well-tempered n-plet dark matter |
title_full |
Well-tempered n-plet dark matter |
title_fullStr |
Well-tempered n-plet dark matter |
title_full_unstemmed |
Well-tempered n-plet dark matter |
title_sort |
well-tempered n-plet dark matter |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2017-09-01 |
description |
Abstract We study simple effective models of fermionic WIMP dark matter, where the dark matter candidate is a mixture of a Standard Model singlet and an n-plet of SU2 L with n ≥ 3, stabilized by a discrete symmetry. The dark matter mass is assumed to be around the electroweak scale, and the mixing is generated by higher-dimensional operators, with a cutoff scale ≳TeV. For appropriate values of the mass parameters and the mixing we find that the observed dark matter relic density can be generated by coannihilation. Direct detection experiments have already excluded large parts of the parameter space, and the next-generation experiments will further constrain these models. |
topic |
Beyond Standard Model Cosmology of Theories beyond the SM |
url |
http://link.springer.com/article/10.1007/JHEP09(2017)160 |
work_keys_str_mv |
AT abharucha welltemperednpletdarkmatter AT fbrummer welltemperednpletdarkmatter AT rruffault welltemperednpletdarkmatter |
_version_ |
1725108911416016896 |