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Phenomenology of the hidden SU(2) vector dark matter model

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dc.creator FAISEL, Gaber
dc.creator Nasri, Salah
dc.creator Baouche, Nabil
dc.creator Ahriche, Amine
dc.date 2021-10-01T00:00:00Z
dc.date.accessioned 2021-12-03T11:31:49Z
dc.date.available 2021-12-03T11:31:49Z
dc.identifier 8abc5e96-45f7-45b2-a5ae-098ee837d185
dc.identifier 10.1103/physrevd.104.075022
dc.identifier https://avesis.sdu.edu.tr/publication/details/8abc5e96-45f7-45b2-a5ae-098ee837d185/oai
dc.identifier.uri http://acikerisim.sdu.edu.tr/xmlui/handle/123456789/93200
dc.description We investigate the phenomenology of an extension of the Standard Model (SM) by a non-Abelian gauge group SU(2)(HS) where all SM particles are singlets under this gauge group, and a new scalar representation phi that is singlet under SM gauge group and doublet under SU(2)(HS). In this model, the dark matter (DM) candidates are the three mass-degenerate dark photons A(i) (i = 1, 2, 3) of SU(2)(HS), and the hidden sector interacts with the (SM) particles through the Higgs portal interactions. Consequently, there will be a new CP-even scalar. that could be either heavier or lighter than the SM-like Higgs. By taking into account all theoretical and experimental constraints such as perturbativity, unitarity, vacuum stability, non-SM Higgs decays, DM direct detection, and M relic density, we found viable DM is possible in the range from GeV to TeV. Within the viable parameters space, both of the triple Higgs coupling and the di-Higgs production at LHC14 could be enhanced or reduced depending on the scalar mixing and the mass of the scalar particle eta.
dc.language eng
dc.rights info:eu-repo/semantics/closedAccess
dc.title Phenomenology of the hidden SU(2) vector dark matter model
dc.type info:eu-repo/semantics/article


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