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• W2271450047 abstract "Herein we use the measurements of the AMS-02 electron flux for the first time in order to derive limits on the dark-matter annihilation cross section and lifetime for the specific final states of ${ensuremath{mu}}^{+}{ensuremath{mu}}^{ensuremath{-}}$ and ${ensuremath{tau}}^{+}{ensuremath{tau}}^{ensuremath{-}}$. With the well-motivated assumption that the electrons were generated from astrophysical processes, we impose strong limits on the dark-matter properties that are insensitive of propagation parameters and nucleon injection parameters when the dark matter particle mass (${m}_{ensuremath{chi}}$) is larger than $ensuremath{sim}200text{ }text{ }mathrm{GeV}$. Specifically, our limits are stronger than those derived from the positron fraction or flux for ${m}_{ensuremath{chi}}g100text{ }text{ }mathrm{GeV}$, and the dark-matter annihilation (or decay) origin of the AMS-02 positron anomaly is found to be disfavored." @default.
• W2271450047 created "2016-06-24" @default.
• W2271450047 creator A5007350077 @default.
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• W2271450047 date "2015-11-13" @default.
• W2271450047 modified "2023-10-17" @default.
• W2271450047 title "Constraints on dark matter from AMS-02 electron data" @default.
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• W2271450047 doi "https://doi.org/10.1103/physrevd.92.103002" @default.
• W2271450047 hasPublicationYear "2015" @default.
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