Electron-Capture Isotopes could Constrain Cosmic-Ray Propagation Models

Abstract

Electron capture (EC) isotopes are known to provide constraints on the low energy behavior of cosmic rays (CRs), such as re-acceleration. Here we study the EC isotopes within the framework of the dynamic spiral-arms CR propagation model in which most of the CR sources reside in the galactic spiral arms. The model was previously used to explain the B/C and sub-Fe/Fe ratios \citep{BoverC,Iron}. We show that the known inconsistency between the ${}^{49}$Ti/${}^{49}$V and ${}^{51}$V/${}^{51}$Cr ratios remains also in the spiral-arms model. On the other hand, unlike the general wisdom in which the isotope ratios depend primarily on reacceleration, we find here that the ratio also depends on the halo size ($z_{\mathrm{h}}$) and in spiral-arms models also on the time since the last spiral arm passage (${\tau }_{\mathrm{arm}}$). Namely, EC isotopes can in principle provide interesting constraints on the diffusion geometry. However, with the present uncertainties in the lab measurements of both the electron attachment rate and the fragmentation cross-sections, no meaningful constraint can be placed.

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Cited by in corpus (2)

• Lower limits on the nucleosynthezis of ${}^{44}$Ti and ${}^{60}$Fe in the dynamic spiral-arms model
• Revisiting electron-capture decay for Galactic cosmic-ray data