Energy concentration in high energy hadron-gamma families

Details Energy concentration in high energy hadron-gamma families Energy concentration in high energy hadron-gamma families

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993eme..work...29t&link_type=abstract

In Tokyo Univ., Contributions to the 23rd ICRC from Emulsion Chamber Experiments at Mt. Chacaltaya and Pamirs p 29-32 (SEE N94-2

Other

Cosmic Ray Showers, Energy Spectra, Hadrons, High Energy Interactions, Nuclear Interactions, Spectral Energy Distribution, Antinucleons, Charged Particles, Flux (Rate), Gamma Rays, Nucleons, Pions

Scientific paper

Exotic hadron-gamma families of 'Centauro-species' were observed and how inclusion of exotic processes changes the relation between family intensity and rate of energy concentration was also studied by constructing simple toy-model for exotic processes. The relations in this model are closer to those of experimental data than in the other models of pion multiple production, but this model gives too many events with very large spread. In the present toy-model, secondary nucleons are assumed to be produced with large pt, and then secondaries and tertiaries are spread out. Moreover gamma-rays are tertiary products and the energy dissipation of gamma-ray component becomes very large, and only those events which make interaction near and above the chamber can be detected. Thus low intensity of family observation together with hard spectrum of showers in the families and high rate of energy concentration indicate that the observed families are in a young stage of atmospheric nuclear cascade development. It is assumed that secondaries in Centauro and mini-Centauro interactions are nucleons and anti-nucleons, and these particles make interaction during passage process through the atmosphere.

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