Alpha particle driven Alfv\'enic instabilities in ITER post-disruption plasmas

Fusion-born alpha particles in ITER disruption simulations are investigated as a possible drive of Alfv\'enic instabilities. The ability of these waves to expel runaway electron (RE) seed particles is explored in the pursuit of a passive, inherent RE mitigation scenario. The spatiotemporal evolution of the alpha particle distribution during the disruption is calculated using the linearized Fokker-Planck solver CODION coupled to a fluid disruption simulation. The radial anisotropy of the resulting alpha population provides free energy to drive Alfv\'enic modes during the quench phase of the disruption. We use the linear gyrokinetic magnetohydrodynamic code LIGKA to calculate the Alfv\'en spectrum and find that the equilibrium is capable of sustaining a wide range of modes. The self-consistent evolution of the mode amplitudes and the alpha distribution is calculated utilizing the wave-particle interaction tool HAGIS. Intermediate mode number ($n=7-15,~22-26$) Toroidal Alfv\'en Eigenmodes (TAEs) are shown to saturate at an amplitude of up to $\delta B /B \approx 0.1$\% in the spatial regimes crucial for RE seed formation. We find that the modes enhance the radial transport of fast electrons which can ultimately reduce or suppress runaway electron generation.