New Calculation of Radioactive Secondaries in Cosmic Rays

Details New Calculation of Radioactive Secondaries in Cosmic Rays New Calculation of Radioactive Secondaries in Cosmic Rays

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0216248m&link_type=abstract

Technical Report, DE2001-783154; LA-UR-01-2982

Mathematics

Cosmic Rays, Mathematical Models, Isotope Ratios, Excitons, Galaxies, Halos

Scientific paper

We use a new version of our numerical model for particle propagation in the galaxy to study radioactive secondaries. For evaluation of the production cross sections we use the Los Alamos compilation of all available experimental cross sections together with calculations using the improved Cascade-Exciton Model code CEM2k. Using the radioactive secondary ratios Al-26/Al-27, Cl-36/Cl, Mn-54/Mn, we show how the improved cross-section calculations together with the new propagation code allow us to better constrain the size of the cosmic ray halo.

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