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Heavy Wino-like Neutralino Dark Matter Annihilation into Antiparticles

Junji Hisano·Shigeki Matsumoto·Osamu Saito·Masato Senami
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Abstract

The lightest neutralino is a viable dark matter (DM) candidate. In this paper we study indirect detection of the wino-like neutralino DM using positrons and antiprotons from the annihilation in the galactic halo. When the mass is around 2 TeV, which is favored from the thermal relic abundance, the non-perturbation effect significantly enhances the annihilation cross sections into positrons and antiprotons. We find that the positron and antiproton fluxes with energies larger than 100 GeV may become larger than the expected backgrounds. Since the positron flux is less sensitive to the astrophysical parameters, the detection may be promising in the upcoming experiments such as PAMELA and AMS-02. We also find the wino-like neutralino DM with mass around 2 TeV is compatible with the HEAT anomaly.

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Junji Hisano, Shigeki Matsumoto, Osamu Saito, Masato Senami. 2006-03-09. Heavy Wino-like Neutralino Dark Matter Annihilation into Antiparticles. https://doi.org/10.1103/physrevd.73.055004

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