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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01rb68xf24b
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dc.contributor.advisorQin, Hongen_US
dc.contributor.authorBurby, Joshua Williamen_US
dc.contributor.otherAstrophysical Sciences Departmenten_US
dc.date.accessioned2015-12-07T19:53:15Z-
dc.date.available2015-12-07T19:53:15Z-
dc.date.issued2015en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01rb68xf24b-
dc.description.abstractHamiltonian structure is pursued and uncovered in collisional and collisionless gyrokinetic theory. A new Hamiltonian formulation of collisionless electromagnetic theory is presented that is ideally suited to implementation on modern supercomputers. The method used to uncover this structure is described in detail and applied to a number of examples, where several well-known plasma models are endowed with a Hamiltonian structure for the first time. The first energy- and momentum-conserving formulation of full-F collisional gyrokinetics is presented. In an effort to understand the theoretical underpinnings of this result at a deeper level, a \emph{stochastic} Hamiltonian modeling approach is presented and applied to pitch angle scattering. Interestingly, the collision operator produced by the Hamiltonian approach is equal to the Lorentz operator plus higher-order terms, but does not exactly conserve energy. Conversely, the classical Lorentz collision operator is provably not Hamiltonian in the stochastic sense.en_US
dc.language.isoenen_US
dc.publisherPrinceton, NJ : Princeton Universityen_US
dc.relation.isformatofThe Mudd Manuscript Library retains one bound copy of each dissertation. Search for these copies in the library's main catalog: http://catalog.princeton.edu/en_US
dc.subjectCollisionsen_US
dc.subjectgyrokineticen_US
dc.subjectHamiltonianen_US
dc.subjectLagrangianen_US
dc.subjectStochasticen_US
dc.subject.classificationPlasma physicsen_US
dc.titleChasing Hamiltonian structure in gyrokinetic theoryen_US
dc.typeAcademic dissertations (Ph.D.)en_US
pu.projectgrantnumber690-2143en_US
Appears in Collections:Plasma Physics

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