Test of the Diffusion Halo and the Leaky Box Model by means of secondary radioactive Cosmic Ray Nuclei with different life times

Details Test of the Diffusion Halo and the Leaky Box Model by means of secondary radioactive Cosmic Ray Nuclei with different life times Test of the Diffusion Halo and the Leaky Box Model by means of secondary radioactive Cosmic Ray Nuclei with different life times

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..211s&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

At this time there are no measurements available on the energy dependence of the surviving fraction of secondary radioactive cosmic ray nuclei. Such a measurement can be used to distinguish between the Leaky Box and the Diffusion Halo Model. Available data gather around 200 MeV/nucleon. We show that these data at a fixed energy can also be used for a model distinction if one makes use of the different lifetimes of the various radioactive nuclei such as 10Be, 26Al and 36Cl.

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