Exceptional composite dark matter

Abstract We study the dark matter phenomenology of non-minimal composite Higgs models with SO(7) broken to the exceptional group $$G_2$$ G 2 . In addition to the Higgs, three pseudo-Nambu–Goldstone bosons arise, one of which is electrically neutral. A parity symmetry is enough to ensure this resonan...

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Main Authors: Guillermo Ballesteros, Adrián Carmona, Mikael Chala
Format: Article
Language:English
Published: SpringerOpen 2017-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-5040-1
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spelling doaj-34db948852d34bb38f24bb5d1854c01b2020-11-24T21:33:54ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-07-0177711810.1140/epjc/s10052-017-5040-1Exceptional composite dark matterGuillermo Ballesteros0Adrián Carmona1Mikael Chala2Institut de Physique Théorique, Université Paris Saclay, CEA, CNRSTheoretical Physics Department, CERNDepartament de Física Tèorica, Universitat de València and IFIC, Universitat de València-CSICAbstract We study the dark matter phenomenology of non-minimal composite Higgs models with SO(7) broken to the exceptional group $$G_2$$ G 2 . In addition to the Higgs, three pseudo-Nambu–Goldstone bosons arise, one of which is electrically neutral. A parity symmetry is enough to ensure this resonance is stable. In fact, if the breaking of the Goldstone symmetry is driven by the fermion sector, this $$\mathbb {Z}_2$$ Z 2 symmetry is automatically unbroken in the electroweak phase. In this case, the relic density, as well as the expected indirect, direct and collider signals are then uniquely determined by the value of the compositeness scale, f. Current experimental bounds allow one to account for a large fraction of the dark matter of the Universe if the dark matter particle is part of an electroweak triplet. The totality of the relic abundance can be accommodated if instead this particle is a composite singlet. In both cases, the scale f and the dark matter mass are of the order of a few TeV.http://link.springer.com/article/10.1140/epjc/s10052-017-5040-1
collection DOAJ
language English
format Article
sources DOAJ
author Guillermo Ballesteros
Adrián Carmona
Mikael Chala
spellingShingle Guillermo Ballesteros
Adrián Carmona
Mikael Chala
Exceptional composite dark matter
European Physical Journal C: Particles and Fields
author_facet Guillermo Ballesteros
Adrián Carmona
Mikael Chala
author_sort Guillermo Ballesteros
title Exceptional composite dark matter
title_short Exceptional composite dark matter
title_full Exceptional composite dark matter
title_fullStr Exceptional composite dark matter
title_full_unstemmed Exceptional composite dark matter
title_sort exceptional composite dark matter
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2017-07-01
description Abstract We study the dark matter phenomenology of non-minimal composite Higgs models with SO(7) broken to the exceptional group $$G_2$$ G 2 . In addition to the Higgs, three pseudo-Nambu–Goldstone bosons arise, one of which is electrically neutral. A parity symmetry is enough to ensure this resonance is stable. In fact, if the breaking of the Goldstone symmetry is driven by the fermion sector, this $$\mathbb {Z}_2$$ Z 2 symmetry is automatically unbroken in the electroweak phase. In this case, the relic density, as well as the expected indirect, direct and collider signals are then uniquely determined by the value of the compositeness scale, f. Current experimental bounds allow one to account for a large fraction of the dark matter of the Universe if the dark matter particle is part of an electroweak triplet. The totality of the relic abundance can be accommodated if instead this particle is a composite singlet. In both cases, the scale f and the dark matter mass are of the order of a few TeV.
url http://link.springer.com/article/10.1140/epjc/s10052-017-5040-1
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