Cosmic-ray composition around 1018 eV

Details Cosmic-ray composition around 1018 eV Cosmic-ray composition around 1018 eV

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..47.1919g&link_type=abstract

Physical Review D (Particles and Fields), Volume 47, Issue 5, 1 March 1993, pp.1919-1932

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87

Cosmic-Ray Interactions, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

We use the depth of maximum distribution as measured by the stereo Fly's Eye detector to study the chemical composition of the primary cosmic radiation between 3×1017 eV and 1019 eV. The analysis depends on the use of simulations to study the response of the detector as well as sensitivity to assumptions about the properties of hadronic interactions that determine cascade development. We find that the incident particles include both heavy nuclei and protons in comparable amounts. The fraction of protons appears to increase at the highest energy explored.

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