Rodríguez E, Bhattacharjee A
Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey, 08543, USA and Princeton Plasma Physics Laboratory, Princeton, New Jersey, 08540, USA.
Phys Rev E. 2021 Jul;104(1-2):015213. doi: 10.1103/PhysRevE.104.015213.
The stellarator as a concept of magnetic confinement fusion requires careful design to confine particles effectively. A design possibility is to equip the magnetic field with a property known as quasisymmetry. Though it is generally believed that a steady-state quasisymmetric equilibrium can only be exact locally (unless the system has a direction of continuous symmetry such as the tokamak), we suggest in this work that a change in the equilibrium paradigm can ameliorate this limitation. We demonstrate that there exists a deep physical connection between quasisymmetry and magnetostatic equilibria with anisotropic pressure, extending beyond the isotropic pressure equilibria commonly considered.
作为磁约束聚变概念的仿星器需要精心设计以有效约束粒子。一种设计可能性是使磁场具备一种称为准对称的特性。尽管人们普遍认为稳态准对称平衡只能在局部精确成立(除非系统具有连续对称性方向,如托卡马克),但我们在这项工作中表明,平衡范式的改变可以改善这一限制。我们证明,准对称与具有各向异性压力的静磁平衡之间存在深刻的物理联系,这一联系超出了通常考虑的各向同性压力平衡。