Limits on deeply penetrating particles in the 10(17) eV cosmic ray flux

Details Limits on deeply penetrating particles in the 10(17) eV cosmic ray flux Limits on deeply penetrating particles in the 10(17) eV cosmic ray flux

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..104b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 104-107 (SEE N85-36066 24-93)

Astronomy and Astrophysics

Astrophysics

1

Corpuscular Radiation, Cosmic Rays, Distribution, Flux, Particle Interactions, Energy Spectra, Flux (Rate), Neutrinos, Primary Cosmic Rays, Quarks

Scientific paper

Deeply penetrating particles in the 10 to the 17th power eV cosmic ray flux were investigated. No such events were found in 8.2 x 10 to the 6th power sec of running time. Limits were set on the following: quark-matter in the primary cosmic ray flux; long-lived, weakly interacting particles produced in p-air collisions; the astrophysical neutrino flux. In particular, the neutrino flux limit at 10 to the 17th power eV implies that z, the red shift of maximum activity is 10 in the model of Hill and Schramm.

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