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arxiv: 0802.3322 · v1 · submitted 2008-02-22 · 🌌 astro-ph

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Environmental limits on the non-resonant cosmic-ray current-driven instability

B. Reville , J.G. Kirk , P. Duffy , S. O'Sullivan
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classification 🌌 astro-ph
keywords instabilitynon-resonantcosmic-raygrowthlimitsbellcalculatedcollisions
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We investigate the so-called non-resonant cosmic-ray streaming instability, first discussed by Bell (2004). The extent to which thermal damping and ion-neutral collisions reduce the growth of this instability is calculated. Limits on the growth of the non-resonant mode in SN1006 and RX J1713.7-3946 are presented.

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