Multiwavelength/Multimessenger constraints on Dark Matter

Details Multiwavelength/Multimessenger constraints on Dark Matter Multiwavelength/Multimessenger constraints on Dark Matter

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nuphs.194...11b&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 194, p. 11-16.

Physics

Nuclear Physics

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Multiwavelength/Multimessenger constraints on Dark Matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multiwavelength/Multimessenger constraints on Dark Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength/Multimessenger constraints on Dark Matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1427908