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| Report/Journal Article | PUBDB-2015-00231 |
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2015
North-Holland Publ.
Amsterdam
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Please use a persistent id in citations: doi:10.1016/j.physletb.2014.12.016
Report No.: DESY-14-168; arXiv:1409.6920
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.
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