Consequences of a high multiplicity model to the muon spectrum at high energies

Details Consequences of a high multiplicity model to the muon spectrum at high energies Consequences of a high multiplicity model to the muon spectrum at high energies

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....7...13g&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 7 (A85-2

Computer Science

Cosmic Rays, High Energy Interactions, Muons, Spectral Energy Distribution, Cosmic Ray Showers, Gamma Rays, Kaons

Scientific paper

A high multiplicity model that takes kaon contribution and
energy-dependent cross sections into account is used to calculate the
muon spectrum above 0.4 TeV. A comparison conducted with a best-estimate
experimental spectrum indicates good agreement, assuming that primary Fe
nuclei dominate above 10 to the 15th eV/nucleon.

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