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

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

2008-02-22

arxiv.org/abs/0802.3322v1

Int.J.Mod.Phys.D17:1795-1801,2008

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, contributed talk at the workshop: High Energy Phenomena in Relativistic Outflows (HEPRO), Dublin, 24-28 Sep

Scientific paper

10.1142/S021827180801342X

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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