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arXiv:1409.6920·v1·High Energy Physics — Phenomenology

Mass of Decaying Wino from AMS-02 2014

Masahiro Ibe🇯🇵 · Shigeki Matsumoto🇯🇵 · Satoshi Shirai🇩🇪 · Tsutomu T. Yanagida🇯🇵

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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.

Comments: 10 pages, 1 figure

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