Comparison of big event with calculations of the air shower development

Astronomy and Astrophysics – Astronomy

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Cosmic Ray Showers, Electron Photon Cascades, Energy Distribution, Energy Spectra, Gamma Ray Bursts, Hadrons, Nucleon-Nucleon Scattering, Charged Particles, Galactic Cosmic Rays, Gamma Ray Astronomy

Scientific paper

The incidence of high energy hadrons and electron-photons in air showers at various stages of development is calculated. Numerical calculation is used to solve the diffusion equation for a nuclear cascade and analytical calculation for cascade shower induced gamma rays. From these calculations, one can get the longitudinal development of the high energy hadron and electron-photon components, and the energy spectra of these components at various depths of air shower development. The total number of hadrons (NH) and electron-photon components (Ngamma) are related according to stages of the air shower development and primary energy. The relation of the total energy of hadron and electron-photon component above the threshold energy is given. The energy balance between both components is also a useful parameter to study high energy events accompanying air showers. The relation of NH and fractional hadronic energy E (sum EHgamma/sum EHgamma + Sum Egamma) is calculated. This relation is helpful to understand the stage of air shower development(t) and primary energy (E sub p).

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