Derivation of vertical muon spectra at superhigh energies from our predicted primary cosmic-ray spectrum using machine interaction parameters and Feynman scaling hypothesis

Details Derivation of vertical muon spectra at superhigh energies from our predicted primary cosmic-ray spectrum using machine interaction parameters and Feynman scaling hypothesis Derivation of vertical muon spectra at superhigh energies from our predicted primary cosmic-ray spectrum using machine interaction parameters and Feynman scaling hypothesis

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ncimc...5..287b&link_type=ejournal

Nuovo Cimento C, Serie 1, vol. 5C, May-June 1982, p. 287-298.

Physics

5

Energy Spectra, High Energy Interactions, Muons, Primary Cosmic Rays, Atmospheric Diffusion, Elementary Particle Interactions, Energetic Particles, Feynman Diagrams, Hadrons, Mesons, Particle Diffusion, Particle Flux Density, Scaling Laws, Vertical Distribution

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