Upper Bounds on Gyrokinetic Instabilities in Magnetized Plasmas

A family of rigorous upper bounds on the growth rate of local gyrokinetic instabilities in magnetized plasmas is derived from the evolution equation for the Helmholtz free energy. These bounds hold for both electrostatic and electromagnetic instabilities, regardless of the number of particle species, their collision frequency, and the geometry of the magnetic field. A large number of results that have earlier been derived in special cases and observed in numerical simulations are thus brought into a unifying framework. These bounds apply not only to linear instabilities but also imply an upper limit to the nonlinear growth of the free energy.

Figure 1

Upper bound [Eq. (11)] on the growth rate (in arbitrary units) of gyrokinetic instabilities for $k_{\psi }=0$ and three different values of $\tau =T_i/T_e$ in a plasma with adiabatic electrons as a function of the smallest value of $k_{\perp }{\rho }_i$ along the magnetic field.