The nonlinear development of the relativistic two-stream instability
The nonlinear development of the relativistic two-stream instability
The two-stream instability has been mooted as an explanation for a range of astrophysical applications from GRBs and pulsar glitches to cosmology. Using the first nonlinear numerical simulations of relativistic multi-species hydrodynamics we show that the onset and initial growth of the instability are very well described by linear perturbation theory. In the later stages the linear and nonlinear description match only qualitatively, and the instability does not saturate even in the nonlinear case by purely ideal hydrodynamic effects.
145007
Hawke, Ian
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Andersson, N.
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Comer, Gregory L
844e5be1-aab1-4406-a5c7-951e4988268f
12 June 2013
Hawke, Ian
fc964672-c794-4260-a972-eaf818e7c9f4
Andersson, N.
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Comer, Gregory L
844e5be1-aab1-4406-a5c7-951e4988268f
Hawke, Ian, Andersson, N. and Comer, Gregory L
(2013)
The nonlinear development of the relativistic two-stream instability.
Classical and Quantum Gravity, 30 (14), .
(doi:10.1088/0264-9381/30/14/145007).
Abstract
The two-stream instability has been mooted as an explanation for a range of astrophysical applications from GRBs and pulsar glitches to cosmology. Using the first nonlinear numerical simulations of relativistic multi-species hydrodynamics we show that the onset and initial growth of the instability are very well described by linear perturbation theory. In the later stages the linear and nonlinear description match only qualitatively, and the instability does not saturate even in the nonlinear case by purely ideal hydrodynamic effects.
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MultiFluid_IOP.pdf
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Published date: 12 June 2013
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Applied Mathematics
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Local EPrints ID: 353665
URI: http://eprints.soton.ac.uk/id/eprint/353665
ISSN: 0264-9381
PURE UUID: c9e98394-f173-4dd1-82e6-d9edf8dfc6a2
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Date deposited: 13 Jun 2013 11:50
Last modified: 15 Mar 2024 03:22
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Gregory L Comer
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