期刊
NUCLEAR PHYSICS B
卷 800, 期 1-2, 页码 204-220出版社
ELSEVIER
DOI: 10.1016/j.nuclphysb.2008.03.013
关键词
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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 can be generated above the background, even with a modest astrophysical boost factor, in the range of energies soon to be explored by cosmic ray experiments. (c) 2008 Elsevier B.V. All rights reserved.
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