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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01ww72bb695
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dc.contributorStaggs, Suzanne-
dc.contributor.advisorBhattacharjee, Amitava-
dc.contributor.authorCarruth, Peter-
dc.date.accessioned2014-07-28T19:52:30Z-
dc.date.available2014-07-28T19:52:30Z-
dc.date.created2014-05-05-
dc.date.issued2014-07-28-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01ww72bb695-
dc.description.abstractThe generation of magnetic fields in plasmas, either astrophysical or in laser experiments, is not well understood. One proposed mechanism is the Biermann battery effect, which goes with \(\nabla\)n\(_{e}\) \(\times\) \(\nabla\)p\(_{e}\) and is derived from a general form of Ohm's law. This effect is derived from fluid mechanics approximations of plasmas, and has not been determined from first principles kinematics. In this thesis, we perform a particle-in-cell simulation of plasma particles and computationally examine this effect. We find that this effect does contribute to magnetic field. We further find that the scalar pressure approximation does not fully cover the magnetic field generation after early simulation times, and by replacing the pressure with the pressure tensor achieve significantly better agreement. This thesis provides one of the first analyses of this effect from kinematics.en_US
dc.format.extent45 pagesen_US
dc.language.isoen_USen_US
dc.titleMagnetic Field Generation and Stability in High-Energy Density Plasmasen_US
dc.typePrinceton University Senior Theses-
pu.date.classyear2014en_US
pu.departmentPhysicsen_US
pu.pdf.coverpageSeniorThesisCoverPage-
Appears in Collections:Physics, 1936-2020

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