Limits on deeply penetrating particles in the >1017 eV cosmic-ray flux

Details Limits on deeply penetrating particles in the >1017 eV cosmic-ray flux Limits on deeply penetrating particles in the >1017 eV cosmic-ray flux

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..31.2192b&link_type=abstract

Physical Review D (Particles and Fields), Volume 31, Issue 9, 1 May 1985, pp.2192-2198

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97

Nuclear Matter

Scientific paper

We report on a search for deeply penetrating particles in the >1017 eV cosmic-ray flux using the University of Utah Fly's Eye detector. No such events have been found in 6×106 sec of running time. We consequently set limits on the following: quark matter in the primary cosmic-ray flux, high-energy long-lived weakly interacting particles produced in proton-air interactions, such as τ's astrophysical neutrino flux; and other hypothetical high-energy weakly interacting components of the cosmic-ray flux such as photinos.

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