Computer Science – Numerical Analysis
Scientific paper
Jan 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jphg....1..120c&link_type=abstract
Journal of Physics, Part G - Nuclear Physics, vol. 1, Jan. 10, 1975, p. 120-133.
Computer Science
Numerical Analysis
5
Cosmic Ray Showers, Electron Distribution, Energy Spectra, Inelastic Scattering, Scattering Cross Sections, Altitude Simulation, Astronomical Models, Electromagnetic Absorption, Electromagnetic Interactions, Electron Photon Cascades, Mean Free Path, Numerical Analysis, Primary Cosmic Rays
Scientific paper
Lateral electron distributions of cosmic extensive air showers (EAS) recorded at energies not greater than 100 TeV are not in agreement with constant inelasticity and constant cross section of ultra-high energy interactions. Theoretical analysis indicates that the p-p cross section and inelasticity are either decreasing together from a maximum larger than 56 mb and 0.55 when the energy is rising from 30 to 100 TeV, or are decreasing separately from higher maximum values.
Cachon A.
Capdevielle Jean-Noel
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