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Electron-capture Isotopes Could Constrain Cosmic-Ray Propagation Models

  • Authors: David Benyamin, Nir J. Shaviv, and Tsvi Piran

2017 The Astrophysical Journal 851 109.

  • Provider: AAS Journals

Caption: Figure 6.

Contour map of the optimal attachment cross-section normalization, N, required to fit the combined ﹩{\chi }^{2}﹩ calculation of the two data sets, as a function of zh and ﹩{\tau }_{\mathrm{arm}}﹩. It is readily seen that the normalization, N, increases when zh increases, while it decreases with ﹩{\tau }_{\mathrm{arm}}﹩. Note that the rugged behavior arises from the raw data having “Monte Carlo” noise.

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