The influence of high-energy electron radiation length on the development of extensive cosmic-ray showers in the atmosphere /10 to the 13th to 10 to the 18th power eV/

Physics

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Cosmic Ray Showers, Electron Photon Cascades, High Energy Electrons, Primary Cosmic Rays, Absorption Spectra, Abundance, Atmospheric Ionization, Atomic Excitations, Muons

Scientific paper

A variation in the calculated value of the high-energy electron
radiation length implies an important modification in the development of
electron photon cascades during extensive showers. This variation
affects the interpretation of experimental values, the evaluation of
energy levels, and the identification of primary cosmic particles.

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