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Intranuclear cascading in photographic emulsion at accelerator and cosmic-ray energies

R. E. Gibbs

J. R. Florian, L. D. Kirkpatrick, J. J. Lord, and J. W. Martin

  • Department of Physics, Eastern Washington State College, Cheney, Washington 99004

  • Department of Physics, University of Washington, Seattle, Washington 98195

Phys. Rev. D 10, 783 – Published 1 August, 1974

DOI: https://doi.org/10.1103/PhysRevD.10.783

Abstract

The data on the interactions of cosmic-ray protons in nuclear emulsion have been analyzed in light of the results of recent exposures of emulsion to accelerator protons. Plots of log10tanθ as a function of the number of evaporation prongs, Nh, display an energy-independent behavior which is exploited to determine the energies of cosmic-ray events. It is found that the energies quoted in the literature are generally too high. The average charged multiplicity is linearly related to Nh from 30 GeV to 5 TeV. While a model of nuclear cascading based on direct production is consistent with these data from 30 GeV to 500 GeV, a model proceeding through an intermediate state gives better agreement at cosmic-ray energies.

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