Article ID Journal Published Year Pages File Type
1851004 Physics Letters B 2015 6 Pages PDF
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

Related Topics
Physical Sciences and Engineering Physics and Astronomy Nuclear and High Energy Physics
Authors
, ,