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Electron acceleration by a relativistic two stream instability with oblique B
Linköping University, Department of Science and Technology, Visual Information Technology and Applications (VITA). Linköping University, The Institute of Technology.ORCID iD: 0000-0003-4055-0552
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
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2006 (English)In: 33rd European Physical Society Conference on Plasma Physics,2006, Rome: European Physical Society , 2006, P4.071- p.Conference paper, Published paper (Refereed)
Abstract [en]

Electrons that are trapped by a quasi-electrostatic wave move, on average, with the phase speed of the wave. In the presence of a magnetic field B, the trapped electrons could, in principle, be accelerated to cosmic ray energies through cross-field transport. We model this cross-field transport with a particle-in-cell (PIC) simulation for an oblique B. The electron energies at the simulation's end exceed 5 MeV for all pitch angles and they can reach GeV energies along the wavevector. We discuss environments, in which such conditions may exist and for which such an acceleration would be relevant.

Place, publisher, year, edition, pages
Rome: European Physical Society , 2006. P4.071- p.
Keyword [en]
plasma physics
National Category
Engineering and Technology
Identifiers
URN: urn:nbn:se:liu:diva-35709Local ID: 28209OAI: oai:DiVA.org:liu-35709DiVA: diva2:256557
Note
ISBN 2-914771-40-1Available from: 2009-10-10 Created: 2009-10-10 Last updated: 2017-11-03

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http://eps2006.frascati.enea.it/papers/start.htm

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Dieckmann, Mark EYnnerman, Anders

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  • en-US
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  • sv-SE
  • Other locale
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