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Production and Propagation of Particles with in the Galaxy
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 () cosmic rays by spallation on interstellar hydrogen in the galaxy. If one takes a single source which suddenly injects particles with an -process charge spectrum years in the past, the calculated relative abundance ratios in four atomic mass groups are consistent with measured values for years. We further conclude that for any initial source distribution the upper limit on is years.
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