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Production and Propagation of Particles with A>81 in the Galaxy

T. B. Kaiser, J. R. Wayland*, and G. Gloeckler

  • Center for Theoretical Physics of the Department of Physics and Astronomy, University of Maryland, College Park, Maryland 20742

  • *Present address: Department of Physics, Texas A&M University, College Station, Texas 77843.
  • Alfred P. Sloan Foundation Fellow.

Phys. Rev. D 5, 307 – Published 15 January, 1972

DOI: https://doi.org/10.1103/PhysRevD.5.307

Abstract

A detailed mathematical model is developed to describe the transformation of the charge composition of superheavy (A>81) cosmic rays by spallation on interstellar hydrogen in the galaxy. If one takes a single source which suddenly injects particles with an r-process charge spectrum t0 years in the past, the calculated relative abundance ratios in four atomic mass groups are consistent with measured values for t02.5×105 years. We further conclude that for any initial source distribution the upper limit on t0 is 106 years.

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