Propagation of cosmic-ray nuclei with reacceleration.

Details Propagation of cosmic-ray nuclei with reacceleration. Propagation of cosmic-ray nuclei with reacceleration.

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hepnp..16..392l&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 16, No. 5, p. 392 - 397

Physics

Scientific paper

Introducing an effective energy change rate of galactic cosmic ray (GCR) during interstellar propagation, the authors obtain a general method of solving the propagation equation of GCR nuclei - the modified slab weighted method. In the leaky box model, they give comparisons of calculated ratios of secondary and primary nuclei and primary energy spectra with observed results.

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