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Trapping of Cosmic Rays in MHD Turbulence

  • Authors: Siyao Xu, and Alex Lazarian

2020 The Astrophysical Journal 894 63.

  • Provider: AAS Journals

Caption: Figure 7.

Same as Figure 6(a), but for PeV CRs. The numerical evaluations of ﹩{{\rm{\Gamma }}}_{s,{\rm{A}}}﹩ and ﹩{{\rm{\Gamma }}}_{s,s}﹩ are obtained by using the numerical calculations of ﹩{D}_{\mu \mu ,\mathrm{QLT},{\rm{A}}}﹩ in Equation (1) and ﹩{D}_{\mu \mu ,\mathrm{QLT},{\rm{s}}}﹩ in Equation (12), respectively.

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