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Minimal Dark Matter predictions for galactic positrons, anti-protons, photons
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Minimal Dark Matter predictions for galactic positrons, anti-protons, photons
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We present the energy spectra of the fluxes of positrons, anti-protons and photons generated by Dark Matter annihilations in our galaxy, as univocally predicted by the model of Minimal Dark Matter. Due to multi-TeV masses and to the Sommerfeld enhancement of the annihilation cross section, distinctive signals are generated above the background, even with a modest astrophysical boost factor, in the range of energies soon to be explored by cosmic ray experiments.
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Cited by 1 Pith paper
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Revisiting the limits on dark matter annihilation cross-section and decay lifetime in light of electron and positron fluxes
Using CALET, AMS-02, DAMPE, HESS, HAWC, GRAPES-3 and CASA-MIA data, this paper derives 95% C.L. constraints on dark matter annihilation and decay up to 10^16 GeV.
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