6533b824fe1ef96bd127ffef
RESEARCH PRODUCT
Dark Matter and the elusive $\mathbf{Z'}$ in a dynamical Inverse Seesaw scenario
Enrique Fernandez MartinezEnrique Fernandez-martinezValentina De RomeriPedro A. N. MachadoViviana NiroJulia GehrleinJulia Gehrleinsubject
PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSpontaneous symmetry breakingDark matterHigh Energy Physics::PhenomenologyInverseFOS: Physical sciencesFermion16. Peace & justice01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesBeyond Standard Modellcsh:QC770-798Neutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino010306 general physicsPhenomenology (particle physics)Bosondescription
The Inverse Seesaw naturally explains the smallness of neutrino masses via an approximate $B-L$ symmetry broken only by a correspondingly small parameter. In this work the possible dynamical generation of the Inverse Seesaw neutrino mass mechanism from the spontaneous breaking of a gauged $U(1)$ $B-L$ symmetry is investigated. Interestingly, the Inverse Seesaw pattern requires a chiral content such that anomaly cancellation predicts the existence of extra fermions belonging to a dark sector with large, non-trivial, charges under the $U(1)$ $B-L$. We investigate the phenomenology associated to these new states and find that one of them is a viable dark matter candidate with mass around the TeV scale, whose interaction with the Standard Model is mediated by the $Z'$ boson associated to the gauged $U(1)$ $B-L$ symmetry. Given the large charges required for anomaly cancellation in the dark sector, the $B-L$ $Z'$ interacts preferentially with this dark sector rather than with the Standard Model. This suppresses the rate at direct detection searches and thus alleviates the constraints on $Z'$-mediated dark matter relic abundance. The collider phenomenology of this elusive $Z'$ is also discussed.
year | journal | country | edition | language |
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2017-07-26 |