Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1851004 | Physics Letters B | 2015 | 6 Pages |
Abstract
Positron excess observed by PAMELA, Fermi and AMS02 may be due to dark matter (DM) pair annihilation or decay dominantly into muons. In this paper, we consider a scenario with thermal fermionic DM (χ ) with mass ∼O(1–2) TeV∼O(1–2) TeV decaying into a dark Higgs (ϕ ) and an active neutrino (νaνa) instead of the SM Higgs boson and νaνa. We first present a renormalizable model for this scenario with local dark U(1)XU(1)X gauge symmetry, in which the DM χ can be thermalized by Higgs portal and the gauge kinetic mixing. Assuming the dark Higgs (ϕ ) mass is in the range 2mμ
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Authors
P. Ko, Yong Tang,