Contribution of an increasing proton-proton cross section to steepening of the cosmic ray energy spectrum

Details Contribution of an increasing proton-proton cross section to steepening of the cosmic ray energy spectrum Contribution of an increasing proton-proton cross section to steepening of the cosmic ray energy spectrum

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jphg....1l...9g&link_type=abstract

Journal of Physics, Part G - Nuclear Physics, vol. 1, Jan. 10, 1975, p. L9-L12. NSF-supported research.

Physics

Nuclear Physics

1

Energy Spectra, Interstellar Matter, Mathematical Models, Primary Cosmic Rays, Proton-Proton Reactions, Scattering Cross Sections, Asymptotes, Continuity Equation, Inelastic Scattering, Particle Collisions, Proton Scattering, Radiation Spectra

Scientific paper

Detailed calculations show that only a part of the steepening observed
to occur at an energy of approximately 4,000 TeV in the cosmic ray
differential spectrum is likely to be attributable to the effects
arising from an increasing proton-nucleus inelastic cross section, even
if the composition in the region of the break is pure iron.

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