Computer Science – Numerical Analysis
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..214g&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 214-217 (SEE N85-34006 22-93)
Computer Science
Numerical Analysis
Chemical Composition, Cosmic Ray Showers, Energy Spectra, Hadrons, Muons, Electromagnetism, Energy Distribution, Mass Spectra, Mathematical Models, Numerical Analysis
Scientific paper
Data obtained from a large set of air shower simulation calculations with use of highly refined hadronic interaction and shower simulation model are presented, in an attempt to solve the problem of primary chemical composition beyond 100,000 GeV total energy. It is rated that high energy hadrons in air showers offer a rather unique primary mass signature and show that the interpretation of high energy muon data is much more ambiguous. Predictions are compared with experimental data.
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