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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

I. V. Moskalenko (NASA/GSFC) , S. G. Mashnik (T16/LANL) , A. W. Strong (MPE , Garching) This is my paper · ORCID
classification astro-phhep-phnucl-exnucl-th
keywords radioactivecalculationscodecrossimprovedmodelpropagationsecondaries
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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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  1. Prediction of lithium isotope fluxes using data-driven production cross sections

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    Adding heavy-progenitor lithium production with cross sections renormalized to measurements removes the AMS-02 lithium excess and predicts 6Li and 7Li fluxes consistent with preliminary data.

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