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Are ultrahigh energy cosmic rays signals of supersymmetry?

We investigate the possibility that cosmic rays of energy larger than the Greisen-Zatsepin-Kuzmin cutoff are not nucleons, but a new stable, massive, hadron that appears in many extensions of the standard model. We focus primarily on the S^0, a uds-gluino bound state. The range of the S^0 through the cosmic background radiation is significantly longer than the range of nucleons, and therefore can originate from sources at cosmoglogical distances.

preprint1997arXivOpen access
Daniel J. H. ChungGlennys R. FarrarEdward W. Kolb
astro-phhep-ph
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Daniel J. H. ChungGlennys R. FarrarEdward W. Kolb

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