Cross section parameterizations for cosmic-ray nuclei. 2: Double nucleon removal

Details Cross section parameterizations for cosmic-ray nuclei. 2: Double nucleon removal Cross section parameterizations for cosmic-ray nuclei. 2: Double nucleon removal

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apjs...90..115n&link_type=abstract

Astrophysical Journal Supplement Series, vol. 90, no. 1, p. 115-117

Statistics

Computation

3

Abundance, Astrophysics, Cosmic Rays, Nuclear Reactions, Nuclei (Nuclear Physics), Nucleons, Parameterization, Removal, Scattering Cross Sections, Computation, Earth Atmosphere, Electromagnetic Interactions, Interstellar Matter, Numerical Analysis, Spacecraft Shielding, Strong Interactions (Field Theory)

Scientific paper

Parameterizations of double nucleon removal from the electromagnetic and strong interactions of cosmic rays with nuclei are presented. These parameterizations are an extension of previous single nucleon removal parameterizations and combined they represent the dominant part of the electromagnetic dissociation encountered by a cosmic ray on its traversal through matter. Such parameterizations should be very useful in studying cosmic-ray transport through the interstellar medium, the Earth's atmosphere, spacecraft walls, and extraterrestrial matter.

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