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The stability problem of the rotation induced electrostatic wave inextragalactic jets is presented. Solving a set of equations describing dynamicsof a relativistic plasma flow of AGN jets, an expression of the instabilityrate has been derived and analyzed for typical values of AGNs. The growth ratewas studied versus the wave length and the inclination angle and it has beenfound that the instability process is much efficient with respect to theaccretion disk evolution, indicating high efficiency of the instability.

Centrifugally driven electrostatic instability in extragalactic jets