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PreprintCC BY 4.0arXiv

Analytic non-axisymmetric 3D MHD equilibria without stellarator symmetry

Abstract

Analytical solutions to the three-dimensional ideal magnetohydrodynamic equilibrium equations (∇ × B⃗) × B⃗ = ∇ p and ∇ · B⃗ = 0 provide benchmarks for stellarator equilibrium codes. Two families of non-axisymmetric solutions were recently discovered by Landreman [arXiv:2609.26742] as counterexamples to Grad's conjecture, but both satisfy stellarator symmetry. Here, we generalize both families by introducing a symmetry-breaking parameter into each of the solutions, resulting in new non-axisymmetric solutions that break stellarator symmetry and reduce to the stellarator symmetric solutions when the newly introduced parameter is set to zero.

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BibTeX
@misc{issan2026analytic,
  title = {{Analytic non-axisymmetric 3D MHD equilibria without stellarator symmetry}},
  author = {Opal Issan and Jonathan Citrin and Matt Landreman and Brendan Tracey},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.07304},
  eprint = {2610.07304},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.07304},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Analytic non-axisymmetric 3D MHD equilibria without stellarator symmetry
AU  - Opal Issan
AU  - Jonathan Citrin
AU  - Matt Landreman
AU  - Brendan Tracey
PY  - 2026
DA  - 2026/10/05
PB  - arXiv
DO  - 10.48550/arxiv.2610.07304
UR  - https://arxiv.org/abs/2610.07304
AB  - Analytical solutions to the three-dimensional ideal magnetohydrodynamic equilibrium equations (∇ × B⃗) × B⃗ = ∇ p and ∇ · B⃗ = 0 provide benchmarks for stellarator equilibrium codes. Two families of non-axisymmetric solutions were recently discovered by Landreman [arXiv:2609.26742] as counterexamples to Grad's conjecture, but both satisfy stellarator symmetry. Here, we generalize both families by introducing a symmetry-breaking parameter into each of the solutions, resulting in new non-axisymmetric solutions that break stellarator symmetry and reduce to the stellarator symmetric solutions when the newly introduced parameter is set to zero.
ER  -