Abundance Ratio of Secondary to Primary Expected from the Boundaryless Galaxy Model

Details Abundance Ratio of Secondary to Primary Expected from the Boundaryless Galaxy Model Abundance Ratio of Secondary to Primary Expected from the Boundaryless Galaxy Model

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.1945h&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

Based on the boundaryless Galaxy model, we present secondary to primary ratio in the high energy region, > 5 GeV/n, where the low energy effect such as ˜ reacceleration and the ionization energy loss is negligible. We fo cus on two data, B/C and sub-Fe(21-23)/iron, and find reasonable parameters repro ducing nicely both data. We discuss also the anisotropy problem in connection with the parameters we estimate here, gas density n, the diffusion coefficient D and soon.

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