Dark Matter and the elusive Z' in a dynamical Inverse Seesaw scenario [electronic resource]

Beyond Standard Model; Neutrino Physics.

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Bibliographic Details
Online Access: Online Access (via OSTI)
Corporate Author: Fermi National Accelerator Laboratory (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : United States. Department of Energy. High Energy Physics Division ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 2017.
Subjects:

MARC

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245 0 0 |a Dark Matter and the elusive Z' in a dynamical Inverse Seesaw scenario  |h [electronic resource] 
260 |a Washington, D.C. :  |b United States. Department of Energy. High Energy Physics Division ;  |a Oak Ridge, Tenn. :  |b distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,  |c 2017. 
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500 |a Published through SciTech Connect. 
500 |a 10/24/2017. 
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500 |a Journal of High Energy Physics (Online) 2017 10 ISSN 1029-8479 AM. 
500 |a Valentina De Romeri; Enrique Fernandez-Martinez; Julia Gehrlein; Pedro A. N. Machado; Viviana Niro. 
520 3 |a 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. Furthermore, the collider phenomenology of this elusive $Z'$ is also discussed. 
520 0 |a Beyond Standard Model; Neutrino Physics. 
536 |b AC02-07CH11359. 
650 7 |a Physics Of Elementary Particles And Fields.  |2 edbsc. 
710 2 |a Fermi National Accelerator Laboratory.  |4 res. 
710 1 |a United States.  |b Department of Energy.  |b High Energy Physics Division.  |4 spn. 
710 1 |a United States.  |b Department of Energy.  |b Office of Scientific and Technical Information.  |4 dst. 
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