Source composition of cosmic rays at high energy

Details Source composition of cosmic rays at high energy Source composition of cosmic rays at high energy

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....2..653j&link_type=abstract

Presented at the 14th Intern. Cosmic Ray Conf., Munich, West Germany, 15-29 Aug., 1975

Computer Science

6

Chemical Composition, Cosmic Rays, High Energy Interactions, Problem Solving, Radiation Sources, Wave Propagation, Approximation, Nucleons, Particle Trajectories

Scientific paper

The source composition of the cosmic ray is usually calculated at an energy of a few GeV per nucleon. Recent measurements have however indicated that the source composition may be energy dependent. In order to give a quantitative answer to this question the source composition at 50 GeV/ nucleon was calculated using an exponential distribution of pathlengths and in the slab approximation. The results obtained at high energy agree very well with the source composition obtained at lower energies, except the abundance of carbon which is significantly lower than the generally accepted value of low energies.

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