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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 4.

Comparison between ﹩{{\rm{\Gamma }}}_{t,f}﹩ and ﹩{{\rm{\Gamma }}}_{s,f}﹩ in compressible MHD turbulence for TeV CRs. The analytical approximations are given by Equations (29), (31), and (41). The numerical calculation of Equation (12) is used for the numerical evaluation of ﹩{{\rm{\Gamma }}}_{s,f}﹩. The vertical dashed line indicates ﹩{\mu }_{\mathrm{cf},{\rm{f}}}﹩, corresponding to Equation (42).

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