Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....4.1375o&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
The energy distribution of produced particles in multiple particle production is formulated empirically based on the data of direct observations by accelerator and cosmicray experiments at 1012 ˜ 1014 eV. The formulated distribution indicates violation of the Feynman scaling law, which was shown to be valid in low energy region of ≤ 1012 eV. That is, the particle density is suppressed in the forward region and enhanced in the central region, compared with the distribution of the Feynman scaling law. Consequences of the formulated distribution, such as multiplicity, inelasticity, etc., are discussed at high energies of ≥ 1015 eV by extrapolation. The distribution is also compared with those of nuclear interaction models which are used widely in simulations of accelerator and cosmic-ray experiments.
Ohsawa Akinori
Shibuya Edison H.
Tamada Masanobu
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