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arXiv · 2507.21003

Optimizing Particle Transport for Enhanced Confinement in Quasi-Isodynamic Stellarators

A. Bañón Navarro·A. Di Siena·F. Jenko·A. Merlo·E. Laude
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Abstract

Despite significant advances in reducing turbulent heat losses, modern quasi-isodynamic (QI) stellarators -- such as Stellaris -- continue to suffer from poor particle confinement, which fundamentally limits their overall performance. Using gyrokinetic simulations within the GENE--Tango framework, we identify suppressed inward thermodiffusion, caused by unfavorable magnetic geometry, as the primary cause. To overcome this limitation, we design a new configuration with a reduced mirror ratio, which enhances the contribution of passing electrons to the inward particle flux. This facilitates the formation of strongly peaked density profiles, suppresses turbulence, and leads to a substantial improvement in confinement. Our optimized configuration achieves nearly a twofold increase in energy confinement compared to Stellaris, highlighting the crucial role of optimizing particle transport in next-generation stellarator designs.

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A. Bañón Navarro, A. Di Siena, F. Jenko, A. Merlo, E. Laude. 2025-07-28. Optimizing Particle Transport for Enhanced Confinement in Quasi-Isodynamic Stellarators. https://arxiv.org/abs/2507.21003

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