Systematic uncertainties on the cosmic-ray transport parameters - Is it possible to reconcile B/C data with δ = 1/3 or δ = 1/2?

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Table 1:

Reference values for the inputs.
Input name	Default value/dependence/set
Gas	$\Sigma=6.17 \times 10^{20}$ cm $^2, \quad f_{\rm H}= 90\%$
Source spectrum	$\eta_{\rm S}=-1, \quad \alpha+\delta=2.65$
K(E) and $K_{\rm pp}(E)$	Slab Alfvén (SA): Eqs. (5) & (6)
Cross-sections	W03 (Webber et al. 2003)
Data	B/C, dataset F $^{\dagger}$

Notes. In subsequent tables of the paper, all results obtained with the default inputs are in italics. $^{(\dagger)}$ 31 data points from IMP7-8, Voyager 1&2, ACE, HEA0-3, Spacelab, and CREAM04.

Source LaTeX | All tables | In the text

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