Nonlinear Alfvén instability simulation and EP transport for ITER reversed shear (steady-state) and monotonic q-profile regimes

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Abstract

The nonlinear evolution and dynamics of energetic particle (EP) driven instabilities in both steady-state (reversed shear q-profile) and monotonic q-profile regimes of ITER are examined using the global gyro-Landau closure model FAR3d. Both neutral beam and alpha components are included, leading to synergistic effects between the two populations. In order to maintain computational feasibility, the present nonlinear simulation includes all toroidal mode numbers ranging from n = 0 to 15. It cannot be excluded that n’s above this range could introduce larger linear growth rates; however, as indicated from the results, the n = 0 to 15 range is sufficient to provide a strong linear drive and significant nonlinear transport effects. While the toroidal mode numbers n = 6 , 13 dominate the linear instability growth phase, nonlinear energy transfers in the saturated phase reverse this trend, leading to the dominance of lower n’s in the saturated phase of the simulation. Zonal flow structure generation and EP density flattening are further consequences of the nonlinear phase. The density profile flattening is caused by collectively driven EP radial transport fluxes, which have non-local characteristics. Instantaneous alpha particle transport fluxes are significant (Γα ∼ 2 × 1020 m-2 s-1) for the reversed shear regime and lower (Γα ∼ 1.1 × 1020 m-2 s-1) for the monotonic q-profile case.

Original languageEnglish
Article number112004
JournalNuclear Fusion
Volume65
Issue number11
DOIs
StatePublished - Nov 1 2025

Funding

This manuscript has been authored by UT-Battelle,: LLC. under Contract No. DE-AC05- 00OR22725 with the U.S. Department of Energy. Also, this work has been supported by under the USDOE Grant DE-FG02-04ER54742 and the Spanish National Research Project No. PID2022-137869OB-I00. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. The Department of Energy will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ). This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 using NERSC Award FES-ERCAP0031638. Assistance is gratefully acknowledged from Nicolai Gorelenkov (PPPL) and A Polevoi (ITER) for preparing the ASTRA simulation profiles used in this study. We would also like to thank Seth Camp of Nvidia for providing helpful assistance in adapting FAR3d to GPU accelerated systems.

Keywords

  • AE
  • ITER
  • MHD
  • energetic particles
  • tokamaks

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