Analysis of the electron component of EAS at observational level 700 G X cm(-2) with a scale breaking interaction model and gammaisation hypothesis

Mathematics – Logic

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Cosmic Ray Showers, Electrons, Gamma Rays, Muons, Secondary Emission, Gamma Ray Absorption, Models, Prediction Analysis Techniques, Secondary Cosmic Rays, Simulation

Scientific paper

Scale breaking model and gammaisation processes for high energies give a correct description of the longitudinal development of extensive air showers (E.A.S.). From the analysis of phenomenological characteristics of E.A.S. at Tien-Shan experiment, it follows that for energies near 10 to the 6 GeV the secondary particle multiplicity increases with energy faster than is predicted by the accepted scale breaking model.

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