Abstract
We investigate the so-called nonresonant 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 nonresonant mode in SN1006 and RX J1713.7-3946 are presented.
| Original language | English |
|---|---|
| Pages (from-to) | 1795-1801 |
| Number of pages | 7 |
| Journal | International journal of modern physics d |
| Volume | 17 |
| Issue number | 10 |
| Publication status | Published - Sept 2008 |
| Event | International Workshop on High Energy Phenomena in Relativistic Outflows - Dublin, Ireland Duration: 24 Sept 2007 → 28 Sept 2007 |
Keywords
- IONIZED MEDIA
- AMPLIFICATION
- DIFFUSIVE SHOCK ACCELERATION
- ENERGY
- magnetic fields
- Cosmic rays
- MOLECULAR CLOUDS
- CONFINEMENT
- MAGNETIC-FIELD
- SUPERNOVA-REMNANTS
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