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New calculation of radioactive secondaries in cosmic rays

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arxiv astro-ph/0106502 v2 pith:QTN4LPGV submitted 2001-06-27 astro-ph hep-phnucl-exnucl-th

New calculation of radioactive secondaries in cosmic rays

I. V. Moskalenko (NASA/GSFC) , S. G. Mashnik (T16/LANL) , A. W. Strong (MPE , Garching) This is my paper
classification astro-ph hep-phnucl-exnucl-th
keywords radioactivecalculationscodecrossimprovedmodelpropagationsecondaries
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 26Al/27Al, 36Cl/Cl, 54Mn/Mn, we show how the improved cross-section calculations together with the new propagation code allow us to better constrain the size of the CR halo.

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