Limits of applicability of theoretical spatial distribution functions for secondary electrons and photons

Details Limits of applicability of theoretical spatial distribution functions for secondary electrons and photons Limits of applicability of theoretical spatial distribution functions for secondary electrons and photons

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q1260b&link_type=abstract

(Mezhdunarodnyi Seminar po Izucheniiu Shirokikh Atmosfernykh Livnei Kosmicheskikh Luchei, Moscow, USSR, Oct. 21-23, 1974.) Akade

Computer Science

Cosmic Ray Showers, Distribution Functions, Electron Photon Cascades, Secondary Cosmic Rays, Spatial Distribution, Elementary Particle Interactions, Nuclear Interactions, Primary Cosmic Rays, Radiation Distribution

Scientific paper

Root-mean-square shifts from the shower axis are calculated for secondary particles with the highest possible energies to investigate the limits of theoretical spatial distribution functions. The calculations are made in approximations of three distribution theories, and the three sets of results are compared. Based on these comparisons, it is shown in which cases the distribution functions derived according to each theory are applicable.

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