Interaction of neutralino dark matter with cosmic rays and PAMELA/ATIC data
High Energy Astrophysical Phenomena
2011-02-01 v1
Abstract
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.
Keywords
Cite
@article{arxiv.1101.5920,
title = {Interaction of neutralino dark matter with cosmic rays and PAMELA/ATIC data},
author = {A. B. Flanchik},
journal= {arXiv preprint arXiv:1101.5920},
year = {2011}
}
Comments
3 pages, 1 figures, poster presented at the conference "High Energy Astrophysics Today and Tomorrow - 2010", December 2010 in Moscow, Russia