| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1847726 | Nuclear Physics B - Proceedings Supplements | 2009 | 6 Pages |
Abstract
We perform a multiwavelength, multimessenger analysis of the Dark Matter intepretation of the rise in the energy spectrum of the positron ratio observed by the PAMELA satellite above 10 GeV, and other cosmic ray measurements. If standard assumptions are made for the distribution of Dark Matter and the propagation of cosmic rays, current DM models cannot explain cosmic ray measurements without violating other observational constraints.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
