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On the non-existence of stepped-pressure equilibria far from symmetry

dc.contributor.authorQu, Zhisong
dc.contributor.authorHudson, S R
dc.contributor.authorDewar, Robert
dc.contributor.authorLoizu, J.
dc.contributor.authorHole, Matthew
dc.date.accessioned2024-04-08T04:53:22Z
dc.date.issued2021-10-25
dc.date.updated2022-11-20T07:16:31Z
dc.description.abstractThe Stepped Pressure Equilibrium Code (SPEC) (Hudson et al 2012 Phys. Plasmas 19 112502) has been successful in the construction of equilibria in 3D configurations that contain a mixture of flux surfaces, islands and chaotic magnetic field lines. In this model, the plasma is sliced into sub-volumes separated by ideal interfaces, and in each volume the magnetic field is a Beltrami field. In the cases where the system is far from possessing a continuous symmetry, such as in stellarators, the existence of solutions to a stepped-pressure equilibrium with given constraints, such as a multi-region relaxed MHD minimum energy state, is not guaranteed but is often taken for granted. Using SPEC, we have studied two different scenarios in which a solution fails to exist in a slab with analytic boundary perturbations. We found that with a large boundary perturbation, a certain interface becomes fractal, corresponding to the break up of a Kolmogorov-Arnold-Moser (KAM) surface. Moreover, an interface can only support a maximum pressure jump while a solution of the magnetic field consistent with the force balance condition can be found. An interface closer to break-up can support a smaller pressure jump. We discovered that the pressure jump can push the interface closer to being non-smooth through force balance, thus significantly decreasing the maximum pressure it can support. Our work shows that a convergence study must be performed on a SPEC equilibrium with interfaces close to break-up. These results may also provide insights into the choice of interfaces and have applications in finding out the maximum pressure a machine can support.en_AU
dc.description.sponsorshipThis research was undertaken with the assistance of resources and services from the National Computational Infrastructure (NCI), which is supported by the Australian Government. This work was supported by a grant from the Simons Foundation/SFARI (560651, AB). This work is partly funded by Australian Research Council Project DP170102606 (Z S Q, R L D, M J H) and by DOE Contract No. DEAC02–76CH03073 (S R H). This work has also been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014–2018 and 2019–2020 under Grant No. 633053 (J L).en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0741-3335en_AU
dc.identifier.urihttp://hdl.handle.net/1885/316578
dc.language.isoen_AUen_AU
dc.publisherInstitute of Physics Publishingen_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP170102606en_AU
dc.rights© 2021 IOP Publishing Ltden_AU
dc.sourcePlasma Physics and Controlled Fusionen_AU
dc.titleOn the non-existence of stepped-pressure equilibria far from symmetryen_AU
dc.typeJournal articleen_AU
dcterms.dateAccepted2021-09-28
local.bibliographicCitation.issue12en_AU
local.contributor.affiliationQu, Zhisong, College of Science, ANUen_AU
local.contributor.affiliationHudson, S R, Princeton Plasma Physics Laboratoryen_AU
local.contributor.affiliationDewar, Robert, College of Science, ANUen_AU
local.contributor.affiliationLoizu, J., Swiss Plasma Centeren_AU
local.contributor.affiliationHole, Matthew, College of Science, ANUen_AU
local.contributor.authoruidQu, Zhisong, u5245081en_AU
local.contributor.authoruidDewar, Robert, u8203580en_AU
local.contributor.authoruidHole, Matthew, u4219046en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.identifier.absfor490105 - Dynamical systems in applicationsen_AU
local.identifier.absfor510602 - Plasma physics; fusion plasmas; electrical dischargesen_AU
local.identifier.absfor490301 - Experimental mathematicsen_AU
local.identifier.ariespublicationa383154xPUB22498en_AU
local.identifier.citationvolume63en_AU
local.identifier.doi10.1088/1361-6587/ac2afcen_AU
local.identifier.scopusID2-s2.0-85118896757
local.identifier.thomsonIDWOS:000711175100001
local.publisher.urlhttps://iopscience.iop.org/en_AU
local.type.statusPublished Versionen_AU

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