The Relativistic Filamentation Instability in Magnetized Plasmas

The Relativistic Filamentation Instability in Magnetized Plasmas

The instability of perpendicular aperiodic fluctuations in a magnetized overall-neutral two-stream distribution function with relativistic speeds is investigated. It is demonstrated that there exists a critical magnetic field strength, above which the filamentation instability is not excited. The th...

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Veröffentlicht in:The Astrophysical journal 2007-04, Vol.659 (1), p.419-425
Hauptverfasser: Stockem, A, Lerche, I, Schlickeiser, R
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Astronomy
Earth, ocean, space
Exact sciences and technology
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creator Stockem, A
Lerche, I
Schlickeiser, R
description The instability of perpendicular aperiodic fluctuations in a magnetized overall-neutral two-stream distribution function with relativistic speeds is investigated. It is demonstrated that there exists a critical magnetic field strength, above which the filamentation instability is not excited. The theory is applied to relativistic jets in AGNs, microquasars, and radio lobes in large radio galaxies.
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Exact sciences and technology
title The Relativistic Filamentation Instability in Magnetized Plasmas
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