Geodesic
Dark matter interpretations of the cosmic-ray $e^\pm$ excesses
Teoretičeskaâ i matematičeskaâ fizika, Tome 170 (2012) no. 2, pp. 248-257 Cet article a éte moissonné depuis la source Math-Net.Ru

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The cosmic-ray excess observed by PAMELA in the positron fraction and by FERMI and HESS in $e^-{+}e^+$ can be interpreted in terms of dark matter annihilations or decays. We summarize the main possibilities and their possible tests.
Keywords: cosmic ray, dark matter
Mots-clés : positron. 
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A. Strumia. Dark matter interpretations of the cosmic-ray $e^\pm$ excesses. Teoretičeskaâ i matematičeskaâ fizika, Tome 170 (2012) no. 2, pp. 248-257. http://geodesic.mathdoc.fr/item/TMF_2012_170_2_a7/

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