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 5:

K(E) and $K_{\rm pp}$ for different schemes.
Type of turbulence		$\eta _{\rm T}$	$\frac{K_{\rm pp} K_{\rm xx}}{4/3~ p^2V_{\rm a}^2}$
LBI	Leaky Box Inspired	0	$\frac{1}{\delta~(4-\delta^2)~(4-\delta)}$
SA	Slab Alfvén	1	$\frac{1}{\delta~(4-\delta^2)~(4-\delta)}$
IFM	Isotropic fast magnetosonic	${2-\delta}$	$\beta^{1-\delta} \ln (\frac{v}{V_{\rm a}})$
Mix	Mixture SA and IFM	${1-\delta}$	$\beta^{1-\delta} \ln (\frac{v}{V_{\rm a}})$

Notes. The spatial diffusion coefficient is $K_{\rm xx}= \beta^{\eta_{\rm T}} \cdot K_0 \cdot {\cal R}^\delta$ .

Source LaTeX | All tables | In the text

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