Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-04
Astronomy and Astrophysics
Astrophysics
7 pages, 4 figures
Scientific paper
10.1063/1.2842365
The stability problem of the rotation induced electrostatic wave in extragalactic jets is presented. Solving a set of equations describing dynamics of a relativistic plasma flow of AGN jets, an expression of the instability rate has been derived and analyzed for typical values of AGNs. The growth rate was studied versus the wave length and the inclination angle and it has been found that the instability process is much efficient with respect to the accretion disk evolution, indicating high efficiency of the instability.
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