Less constrained omnigeneous stellarators
Felix I. Parra, Ivan Calvo, Per Helander, Matt Landreman

TL;DR
This paper broadens the understanding of omnigeneous stellarators by showing that magnetic fields with varying local minima and maxima can still be omnigeneous, expanding the design possibilities beyond previous constraints.
Contribution
It demonstrates that the conditions for omnigeneity are less restrictive than previously thought, allowing for more diverse magnetic field configurations.
Findings
Omnigeneous magnetic fields can have different values at local minima and maxima.
The parameter space for designing omnigeneous stellarators is larger than previously believed.
Improved neoclassical confinement may enhance energetic particle confinement.
Abstract
A stellarator is said to be omnigeneous if all particles have vanishing average radial drifts. In omnigeneous stellarators, particles are perfectly confined in the absence of turbulence and collisions, whereas in non-omnigeneous configurations, particle can drift large radial distances. One of the consequences of omnigeneity is that the unfavorable inverse scaling with collisionality of the stellarator neoclassical fluxes disappears. In the pioneering and influential article [Cary~J~R and Shasharina~S~G 1997 {\it Phys. Plasmas} {\bf 4} 3323], the conditions that the magnetic field of a stellarator must satisfy to be omnigeneous are derived. However, reference [Cary~J~R and Shasharina~S~G 1997 {\it Phys. Plasmas} {\bf 4} 3323] only considered omnigeneous stellarators in which all the minima of the magnetic field strength on a flux surface must have the same value. The same is assumed for…
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