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Wakefield generation in magnetized plasmas

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dc.contributor.author Holkundkar, Amol R.
dc.date.accessioned 2024-01-23T10:14:22Z
dc.date.available 2024-01-23T10:14:22Z
dc.date.issued 2011-09
dc.identifier.uri https://journals.aps.org/pre/abstract/10.1103/PhysRevE.84.036409
dc.identifier.uri http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/13935
dc.description.abstract We consider wakefield generation in plasmas by electromagnetic pulses propagating perpendicular to a strong magnetic field, in the regime where the electron cyclotron frequency is equal to or larger than the plasma frequency. Particle-in-cell simulations reveal that for moderate magnetic field strengths previous results are reproduced, and the wakefield wave number spectrum has a clear peak at the inverse skin depth. However, when the cyclotron frequency is significantly larger than the plasma frequency, the wakefield spectrum becomes broadband, and simultaneously the loss rate of the driving pulse is much enhanced. A set of equations for the scalar and vector potentials reproducing these results are derived, using only the assumption of a weakly nonlinear interaction. en_US
dc.language.iso en en_US
dc.publisher APS en_US
dc.subject Physics en_US
dc.subject Wakefield en_US
dc.subject Magnetized plate en_US
dc.subject Plasma devices en_US
dc.subject Electromagnetic pulses en_US
dc.title Wakefield generation in magnetized plasmas en_US
dc.type Article en_US


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