Analytical solution of 3-D cosmic-ray diffusion in the galaxy with boundaryless halo (III) secondary components -

Details Analytical solution of 3-D cosmic-ray diffusion in the galaxy with boundaryless halo (III) secondary components - Analytical solution of 3-D cosmic-ray diffusion in the galaxy with boundaryless halo (III) secondary components -

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....5.1908s&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Based on the solution of three dimensional cosmic-ray diffusion for the primary component derived by the author, taking a rather realistic structure of our Galaxy into account, we show an analytical solution of the cosmic-ray diffusion for secondary components, typically for Li-Be-B mainly coming from C and O, and for sub-Fe coming from Fe. We present also the solution for unstable nuclei, typically 10 Be.

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