Physics – Nuclear Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ncimb..27..263a&link_type=abstract
Nuovo Cimento, Sezione B, vol. 27 B, June 11, 1975, p. 263-282. Research supported by the Universidad Mayor de San Andres, Organ
Physics
Nuclear Physics
4
Energy Spectra, High Energy Interactions, Nuclear Interactions, Particle Collisions, Primary Cosmic Rays, Proton Energy, Charged Particles, Cosmic Ray Showers, Extrapolation, Nuclei (Nuclear Physics), Proton Impact, Scattering Cross Sections
Scientific paper
The energy spectrum of surviving collisionless primary cosmic-ray protons in the atmosphere has been obtained from the observation of high-energy nuclear bursts produced by singly charged particles in the energy range from 3 TeV to 30 TeV without accompanying air shower particles at Chacaltaya, Bolivia. Comparison of this spectrum with an extrapolation of the energy spectrum of primary cosmic-ray protons obtained by Ryan et al. to higher energies with the same exponent shows a logarithmic rise of the cross-section for proton-air nucleus collisions from 3 TeV to 9 TeV.
Aguirre Carlos
Kamata Kumiko
MacKeown Kevin P.
Maeda Toshihisa
Mejia G. R.
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