Multimuons events and primary composition

Details Multimuons events and primary composition Multimuons events and primary composition

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8....8a&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 8 p 8-11 (SEE N85-36066 24-93)

Mathematics

Probability

Monte Carlo Method, Muons, Primary Cosmic Rays, Radiation Detectors, Atmospheric Density, Heavy Nuclei, Radioactive Decay, Scattering Cross Sections, Simulation

Scientific paper

Nucleon decay detectors at large depths offers now a total area larger than 1000 sq m to registrate muons of energy exceeding 1 TeV. Near complete high energy muon families are detected in those arrays. An extensive 3D Monte-Carlo simulation was conducted in view to understand the spatial distribution of those events and the possible link with elementary act or primary composition. As pion or kaon parents have a very small decay probability at so high energy, multimuon phenomena occurs at high altitude where the atmospheric density is small after the most energetic collisions.

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