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arXiv · 2102.00334

Cosmic-ray current-driven instabilities -- revisiting environmental conditions

B. Reville·G. Giacinti·R. Scott
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Abstract

The growth of magneto-hydrodynamic fluctuations relevant to cosmic ray confinement in and near their sources, and the effects of local plasma conditions is revisited. We consider cases where cosmic rays penetrate a medium which may contain a fraction of neutral particles, and explore the possible effects of high-order cosmic-ray anisotropies. An algorithm for calculating the dispersion relation for arbitrary distributions, and anisotropies is presented, and a general solution for power-law cosmic-ray distributions is provided. Implications for the resulting instabilities near to strong Galactic cosmic-ray sources are discussed. We argue that cosmic-ray streaming in weakly ionised plasmas eliminates the need for the existence of an evanescent band in the dispersion relation, a conclusion which may be confirmed by gamma-ray observations. The necessity for additional multi-scale numerical simulations is highlighted, as understanding the non-linear behaviour is crucial.

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B. Reville, G. Giacinti, R. Scott. 2021-01-30. Cosmic-ray current-driven instabilities -- revisiting environmental conditions. https://doi.org/10.1093/mnras%2Fstab296

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