Superheavy Dark Matter

Details Superheavy Dark Matter Superheavy Dark Matter

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005idm..conf..575k&link_type=abstract

THE IDENTIFICATION OF DARK MATTER. Proceedings of the Fifth International Workshop. Held 6-10 September 2004 in Edinburgh, UK. E

Physics

Scientific paper

Superheavy particles are produced at the end of inflation and could, for a likely set of parameters (e.g. mass MX ~ 1013 GeV and reheating temperature TR ~ 109 GeV), constitute the main part of dark matter. If they are metastable, their decay products may dominate the ultra-high energy cosmic ray flux above ~ 8 × 1019 eV. The main signatures of this scenario, galactic anisotropy and photon dominance, should allow the Auger experiment to test this hypothesis conclusively within one year of data taking.

Affiliated with

Also associated with

No associations

Rating

Superheavy 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 Superheavy Dark Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Superheavy Dark Matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-976094