Quasisymmetry
In magnetic confinement fusion, quasisymmetry (sometimes hyphenated as quasi-symmetry) is a type of continuous symmetry in the magnetic field strength of a stellarator.[1] Quasisymmetry is desired, as Noether's theorem implies that there exists a conserved quantity in such cases. This conserved quantity ensures that particles stick to the flux surface, resulting in better confinement and neoclassical transport.
It is currently unknown if it is mathematically possible to construct a quasi-symmetric magnetic field which upholds magnetohydrodynamic force balance, which is required for stability. There are stellarator designs which are very close to being quasisymmetric,[2] and it is possible to find solutions by generalizing the magnetohydrodynamic force balance equation.[3] Quasisymmetric systems are a subset of omnigenous systems. The Helically Symmetric eXperiment and the National Compact Stellarator Experiment are designed to be quasisymmetric.[citation needed]
References
- ↑ Boozer, Allen H. (1983). "Transport and isomorphic equilibria" (in en). Physics of Fluids 26 (2): 496. doi:10.1063/1.864166. Bibcode: 1983PhFl...26..496B. https://aip.scitation.org/doi/10.1063/1.864166.
- ↑ Landreman, Matt; Paul, Elizabeth (18 January 2022). "Magnetic Fields with Precise Quasisymmetry for Plasma Confinement". Physical Review Letters 128 (3): 035001. doi:10.1103/PhysRevLett.128.035001. PMID 35119901. Bibcode: 2022PhRvL.128c5001L. https://link.aps.org/doi/10.1103/PhysRevLett.128.035001.
- ↑ Rodríguez, E.; Bhattacharjee, A. (January 2021). "Solving the problem of overdetermination of quasisymmetric equilibrium solutions by near-axis expansions. I. Generalized force balance" (in en). Physics of Plasmas 28 (1): 012508. doi:10.1063/5.0027574. ISSN 1070-664X. Bibcode: 2021PhPl...28a2508R. http://aip.scitation.org/doi/10.1063/5.0027574.
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