Diffusion of cosmic rays in MHD turbulence

被引：0

作者：

Xu, Siyao ^{[1
]}

机构：

[1] Inst Adv Study, 1 Einstein Dr, Princeton, NJ 08540 USA

来源：

37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021 | 2022年

关键词：

COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE; GALAXY CLUSTERS; PROPAGATION; ANISOTROPY; TRANSPORT; RECONNECTION; SCATTERING; PARTICLES; SPECTRUM; WAVES;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review some recent findings on diffusion of cosmic rays (CRs) in magnetohydrodynamic (MHD) turbulence obtained by adopting the numerically-tested model of MHD turbulence, including perpendicular superdiffusion of CRs, inefficient gyroresonant scattering by Alfven and slow modes with scale-dependent turbulence anisotropy, resonance-broadened Transit Time Damping (TTD) interaction, and mirror diffusion. As the diffusion behavior of CRs strongly depends on the properties of MHD turbulence, theoretical modeling of CR diffusion, its numerical testing, and interpretation of CR-related observations require proper modeling of MHD turbulence.

引用

页数：16

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