A study of certain characteristics of gamma families with primary particle energies above 10 to the 15th eV

Details A study of certain characteristics of gamma families with primary particle energies above 10 to the 15th eV A study of certain characteristics of gamma families with primary particle energies above 10 to the 15th eV

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55..641m&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, USSR, Nov. 1-3, 1990) Akademiia Nauk SSSR, Izvestiia, Seriia Fizich

Computer Science

Energetic Particles, Gamma Rays, Particle Energy, Primary Cosmic Rays, Cerenkov Counters, Photographic Emulsions, Strong Interactions (Field Theory)

Scientific paper

A study is made of the characteristics of narrow gamma families detected
by X-ray emulsion chambers during the Pamir experiment. The results
obtained are compared with different models of strong interaction. The
fraction of narrow families in the experiment is shown to be sensitive
to the strong-interaction model.

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