Interaction of neutralino dark matter with cosmic rays and PAMELA/ATIC data

Details Interaction of neutralino dark matter with cosmic rays and PAMELA/ATIC data Interaction of neutralino dark matter with cosmic rays and PAMELA/ATIC data

2011-01-31

arxiv.org/abs/1101.5920v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

3 pages, 1 figures, poster presented at the conference "High Energy Astrophysics Today and Tomorrow - 2010", December 2010 in

Scientific paper

The data recently obtained by PAMELA and ATIC show the presence of the peak
in the cosmic positron spectrum at energies above 100 GeV. In this paper it has
been shown that the peak can arise due to processes of the interaction of
cosmic rays with neutralino dark matter, which are accompanied by chargino
production and its leptonic decay.

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