SUSY In The Sky: Observing Ultra-High Energy Cosmic Neutralinos

Details SUSY In The Sky: Observing Ultra-High Energy Cosmic Neutralinos SUSY In The Sky: Observing Ultra-High Energy Cosmic Neutralinos

2002-07-10

arxiv.org/abs/hep-ph/0207133v2

Phys.Lett. B563 (2003) 132-139

Physics

High Energy Physics

High Energy Physics - Phenomenology

version accepted by PLB

Scientific paper

10.1016/S0370-2693(03)00642-7

In models where the ultra-high energy cosmic ray problem is solved by top-down scenarios, a significant flux of ultra-high energy neutralinos is predicted. We calculate the number of events expected from such particles in future experiments such as EUSO or OWL. We show that by using the Earth as a filter, showers generated by neutralinos can be separated from neutrino generated showers. We find that for many models, observable rates are expected.

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