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Monday, May 4, 2009
4:00 AM
335 West Hall
Speaker: Yukio Tomozawa, University of Michigan
This is a review of my work in 1985, which predicted the Pierre Auger Project data showing a correlation between high energy cosmic rays and the locations of AGN. The proposed model suggests a new mass scale at the knee energy in the cosmic ray energy spectrum. If that corresponds to a weakly interacting particle, it suggests the existence of a dark matter particle. A suggestion has been put forward to detect such a particle in a cosmic ray experiment utilizing a large accelerator detector.