High-energy multiple muons and heavy primary cosmic-rays

Details High-energy multiple muons and heavy primary cosmic-rays High-energy multiple muons and heavy primary cosmic-rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..222m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 222-225 (SEE N85-34006 22-93)

Computer Science

Numerical Analysis

Charged Particles, Energy Spectra, Heavy Nuclei, High Energy Interactions, Muons, Primary Cosmic Rays, Elementary Particles, Energy Distribution, Numerical Analysis

Scientific paper

Three-dimensional simulations have been carried out on high-energy multiple muons. On their lateral spread, the comparison with the deep-underground observations so far indicates that the primary cosmic rays seems to include heavy nuclei of high content. The calculated results also suggest a method to determine the average mass number of primary particles in the energy around 1015eV.

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