Article ID Journal Published Year Pages File Type
1850991 Physics Letters B 2015 4 Pages PDF
Abstract

We revisit the decaying wino dark matter scenario in the light of the updated positron fraction, electron and positron fluxes in cosmic ray recently reported by the AMS-02 collaboration. We show the AMS-02 results favor the mass of the wino dark matter at around a few TeV, which is consistent with the prediction on the wino mass in the pure gravity mediation model.

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