Stochastic space-time and the primary energy spectrum of cosmic rays at E(0) greater than or equal to 10 to the 19th eV

Details Stochastic space-time and the primary energy spectrum of cosmic rays at E(0) greater than or equal to 10 to the 19th eV Stochastic space-time and the primary energy spectrum of cosmic rays at E(0) greater than or equal to 10 to the 19th eV

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ncimc...8..531s&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 8 C, Sept.-Oct. 1985, p. 531-537.

Computer Science

2

Energy Spectra, High Energy Interactions, Primary Cosmic Rays, Proton Energy, Space-Time Functions, Stochastic Processes, Elementary Particle Interactions, Galactic Cosmic Rays, Hadrons

Scientific paper

The energy spectrum of primary protons at E(0) greater than or equal to 10 to the 19th eV, i.e., the steepening around 10 to the 19th eV can be explained within the framework of stochastic space-time. Moreover, the complete cutoff of UHCR (ultrahigh-energy cosmic-ray) spectrum can also be avoided and a flattening is favored without considering the extragalactic component of cosmic rays.

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