Environmental limits on the nonresonant cosmic-ray current-driven instability

B. Reville; J. G. Kirk; P. Duffy; S. O'Sullivan

doi:10.1142/S021827180801342X

Environmental limits on the nonresonant cosmic-ray current-driven instability

B. Reville, J. G. Kirk, P. Duffy, S. O'Sullivan

Research output: Contribution to journal › Article › peer-review

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
DOIs	https://doi.org/10.1142/S021827180801342X
Publication status	Published - Sep 2008
Externally published	Yes

Keywords

Cosmic rays
Magnetic fields

Access to Document

10.1142/S021827180801342X

https://arrow.tudublin.ie/scschmatart/163Licence: CC BY-NC-SA

Cite this

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title = "Environmental limits on the nonresonant cosmic-ray current-driven instability",

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.",

keywords = "Cosmic rays, Magnetic fields",

author = "B. Reville and Kirk, \{J. G.\} and P. Duffy and S. O'Sullivan",

year = "2008",

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T1 - Environmental limits on the nonresonant cosmic-ray current-driven instability

AU - Reville, B.

AU - Kirk, J. G.

AU - Duffy, P.

AU - O'Sullivan, S.

PY - 2008/9

Y1 - 2008/9

N2 - 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.

AB - 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.

KW - Cosmic rays

KW - Magnetic fields

UR - https://www.scopus.com/pages/publications/56749151635

U2 - 10.1142/S021827180801342X

DO - 10.1142/S021827180801342X

M3 - Article

SN - 0218-2718

VL - 17

SP - 1795

EP - 1801

JO - International Journal of Modern Physics D

JF - International Journal of Modern Physics D

IS - 10

ER -