Threshold scaling breakdown at energies of 10 exp 16 eV and its possible implications in astrophysics

Details Threshold scaling breakdown at energies of 10 exp 16 eV and its possible implications in astrophysics Threshold scaling breakdown at energies of 10 exp 16 eV and its possible implications in astrophysics

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...15a&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 15-17.

Physics

Cosmic Ray Showers, Elementary Particle Interactions, Energy Spectra, Hadrons, Energetic Particles, Secondary Cosmic Rays

Scientific paper

Results of the Hadron experiments are briefly reviewed. A study of the spectra of EAS core particles with the highest energies indicates an abrupt threshold-type softening of the particles at an energy of 10 exp 16 eV. The disappearance of the fragmentation region of secondary particles may indicate the presence of new multiple generation channels at energies above 5 x 10 exp 15 eV. As a result, about half of primary energy is not detected and/or dissipated in the atmosphere.

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