Abstract
Abstract
The nature of dark matter (DM) and how it may interact with the various fields of the Standard Model (SM) remains a mystery. In this paper we show that the interaction between new light dark matter mediators and the SM particles can be naturally suppressed if one employs a single, flat extra dimension (ED). In this setup, the SM fields are localized in a finite width ‘fat’ brane, similar to models of Universal Extra Dimensions (UED), while DM, in turn, is confined to a thin brane at the opposite end of the ED interval. Including brane localized kinetic terms on the fat brane for the mediator fields, the resulting coupling between the SM and these light mediators can be several orders of magnitude smaller than the corresponding ones between the mediators and DM which we assume to be a typical gauge coupling. We investigate the implications of this scenario for both vector (i.e, dark photon, DP) and scalar mediator fields in the 5-D bulk. In this setup kinetic mixing, which is usually employed to suppress light mediator couplings, is not required. Here we assume that the SM particles couple to the DP via their B − L charges while the DP couples to the DM via a dark charge. Both the vector DP couplings and the corresponding Higgs portal couplings with the SM are shown to be natural small in magnitude with a size dependent on ratio of the 5-D compactification radius, R
−1 ∼ 0.1-1 GeV, and the SM brane thickness, L
−1 ∼ 2-10 TeV, a range chosen to avoid LHC and other experimental constraints. In this framework one can obtain the observed value of the DM relic abundance for a wide range of parameter choices, while the constrains due to direct DM detection and the invisible width of the Higgs do not impose significant challenges to the model. Finally, this mechanism can lead to distinct signatures in both present and upcoming experiments as it combines some common features of UED and DP models in a single ED setup.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Reference102 articles.
1. G. Arcadi et al., The waning of the WIMP? A review of models, searches and constraints, Eur. Phys. J.
C 78 (2018) 203 [arXiv:1703.07364] [INSPIRE].
2. M. Battaglieri et al., US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report, in U.S. Cosmic Visions: New Ideas in Dark Matter, College Park, MD, U.S.A., March 23-25, 2017 (2017) [arXiv:1707.04591] [INSPIRE].
3. D. Feldman, B. Körs and P. Nath, Extra-weakly Interacting Dark Matter, Phys. Rev.
D 75 (2007) 023503 [hep-ph/0610133] [INSPIRE].
4. D. Feldman, Z. Liu and P. Nath, The Stueckelberg Z-prime Extension with Kinetic Mixing and Milli-Charged Dark Matter From the Hidden Sector, Phys. Rev.
D 75 (2007) 115001 [hep-ph/0702123] [INSPIRE].
5. M. Pospelov, A. Ritz and M.B. Voloshin, Secluded WIMP Dark Matter, Phys. Lett.
B 662 (2008) 53 [arXiv:0711.4866] [INSPIRE].
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