Implications of the first AMS-02 measurement for dark matter annihilation and decay
Hong-Bo Jin, Yue-Liang Wu, Yu-Feng Zhou

TL;DR
This paper analyzes recent cosmic ray data from AMS-02, PAMELA, and Fermi-LAT to explore dark matter annihilation and decay models, finding that annihilation into tau leptons best fits the data and that current observations favor annihilation over decay.
Contribution
It provides a comprehensive global analysis of dark matter interpretations of cosmic ray data, considering various propagation models and leptonic channels, and identifies preferred dark matter mass ranges and annihilation channels.
Findings
AMS-02 data favors ~500 GeV DM mass for 2μ final states.
Tension exists between AMS-02 and Fermi-LAT data at high confidence.
Annihilation into tau leptons better explains the data than decay scenarios.
Abstract
In light of the first measurement of the positron fraction by the AMS-02 experiment, we perform a detailed global analysis on the interpretation of the latest data of PAMELA, Fermi-LAT, and AMS-02 in terms of dark matter (DM) annihilation and decay in various propagation models. The allowed regions for the DM particle mass and annihilation cross section or decay life-time are obtained for channels with leptonic final states: , , , , and . We show that for the conventional astrophysical background the AMS-02 positron fraction data alone favour a DM particle mass GeV if DM particles annihilate dominantly into final states, which is significantly lower than that favoured by the Fermi-LAT data of the total flux of electrons and positrons. The allowed regions by the two experiments do not overlap at a high confidence level…
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