Possibility of investigating pion-nucleus interactions at energies above 10 to the 14th eV

Details Possibility of investigating pion-nucleus interactions at energies above 10 to the 14th eV Possibility of investigating pion-nucleus interactions at energies above 10 to the 14th eV

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2137a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Tbilisi, Georgian SSR, Apr. 1986) Akademiia Nauk SSSR, Izvestiia, Seriia Fiz

Astronomy and Astrophysics

Astronomy

Gamma Ray Astronomy, High Energy Interactions, Nuclear Interactions, Pions, Angular Distribution, Electron Photon Cascades, Scaling Laws

Scientific paper

Gamma-families formed in nucleon-nucleus interactions are distinguished from those formed in pion-nucleus interactions on the basis of criteria obtained from scaling-model calculations. The analysis included 906 gamma-families with energies of 30-500 TeV, with a particle number not less than 3 and a minimum electron-photon-cascade energy of 2 TeV. The spatial characteristics of the pion and nucleus families are investigated along with the angular distribution of the gamma-families.

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