Analysis of the spatial-energy characteristics at the periphery of large gamma-families (Sigma E-gamma = 300-1000 TeV)

Details Analysis of the spatial-energy characteristics at the periphery of large gamma-families (Sigma E-gamma = 300-1000 TeV) Analysis of the spatial-energy characteristics at the periphery of large gamma-families (Sigma E-gamma = 300-1000 TeV)

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2132b&link_type=abstract

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

Physics

Nuclear Physics

Gamma Ray Astronomy, Particle Energy, Spatial Distribution, Electron Photon Cascades, Nuclei (Nuclear Physics), Scaling Laws, String Theory

Scientific paper

The lg R-gamma distribution at R-gamma greater than 1 is shown to be sensitive to the interaction model. Of the models considered, the best agreement with experiment at R-gamma greater than 1 is given by a model with the generation of quark-gluon strings and scaling violation in the fragmentation region. The value of Sigma E-gamma R-gamma correlates strongly with energy E0, making it possible to determine E0 from the measured Sigma E-gamma R-gamma with an uncertainty of about 2.

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