Results obtained with X-ray emulsion chambers and their comparison with accelerator data

Details Results obtained with X-ray emulsion chambers and their comparison with accelerator data Results obtained with X-ray emulsion chambers and their comparison with accelerator data

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989izssr..53..260a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Astronomy and Astrophysics

Astrophysics

Cosmic Rays, Nuclear Astrophysics, Nuclear Interactions, Test Chambers, Nuclear Emulsions, Secondary Emission, Velocity Distribution

Scientific paper

X-ray emulsion chamber data on nuclear interactions of cosmic ray particles are compared with accelerator data. It is shown that the rapidity distribution of gamma rays from hadron-nucelus interactions agree well with rapidity distributions of charged secondary particles from interactions between protons and atomic nuclei of the emulsion at proton energies of 400 and 800 GeV. This points to the absence of the drastic breakdown of Feynmann scaling in the fragmentation region as the primary energy ranges from 0.4 to 20 TeV. Data are also presented which demonstrate the conservation of scaling in the fragmentation region in the 20-400 TeV range.

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