Propagation of heavy cosmic-ray nuclei

Details Propagation of heavy cosmic-ray nuclei Propagation of heavy cosmic-ray nuclei

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apjs...56..369l&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 56, Nov. 1984, p. 369-391. Navy-NASA-supported research.

Statistics

Computation

28

Abundance, Cosmic Rays, Electron Capture, Heavy Nuclei, Nuclear Fusion, Particle Acceleration, Integral Equations, Interstellar Space, Linear Equations, Solar System

Scientific paper

Techniques for modeling the propagation of heavy cosmic-ray nuclei, and the required atomic and nuclear data, are assembled in this paper. Emphasis is on understanding nuclear composition in the charge range 3 < Z < 83. Details of the application of "matrix methods" above a few hundred MeV per nucleon, a new treatment of electron capture decay, and a new table of cosmic-ray - stable isotopes are presented. Computation of nuclear fragmentation cross sections, stopping power, and electron stripping and attachment are briefly reviewed.

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