Interpreting cosmic ray spectra and composition above 100 TeV

Details Interpreting cosmic ray spectra and composition above 100 TeV Interpreting cosmic ray spectra and composition above 100 TeV

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..338..855g&link_type=abstract

The 5th conference on the intersections of particle and nuclear physics. AIP Conference Proceedings, Volume 338, pp. 855-862 (1

Other

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

Scientific paper

Cosmic radiation which have energies above 100 TeV are discussed. Exam of the possible sources of such high energy particles are given. Also, measurement of high energy muons in air showers as a probe of composition in the 1014 to 1017 eV region of the spectrum is discussed. Finally, a description of a simulation used to analyze the 1017 to 1019 eV energy region of the spectrum is given. In this higher energy region evidence for a transition to a new population of particles exists. (AIP) ©American Institute of Physics 1995

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