An investigation of mass composition of ultra-high energy cosmic rays with energies above 1019 eV via the study of extensive air showers
2012
The electron and muon components of extensive air shower (EAS) with energies
above 1019 eV are analyzed via various giant EAS arrays. A varying property
of showers is observed for two energy ranges; higher and lower than (3 − 4) x
1019 eV. The age parameter, zenith angle, shower size dependence on muon size
and shower size dependence on primary energy show an increment of mass
composition (MC) above (3−4)x 1019eV. Comparison of the observed EAS results
with the simulations of Capdevielle et al. (2000) and Shinozaki et al. (2005)
gives at most 20% photon fraction for primary energies above 1019 eV. The
arrival directions of showers above 4x1019 eV indicate an increasing
concentration towards the super galactic plane.
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