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Magnetic agnetic field generation in core-sheath jets via the kinetic Kelvin-Helmholtz instability

  • We have investigated magnetic field generation in velocity shears via the kinetic Kelvin-Helmholtz instability (kKHI) using a relativistic plasma jet core and stationary plasma sheath. Our three-dimensional particle-in-cell simulations consider plasma jet cores with Lorentz factors of 1.5, 5, and 15 for both electron-proton and electron-positron plasmas. For electron-proton plasmas, we find generation of strong large-scale DC currents and magnetic fields that extend over the entire shear surface and reach thicknesses of a few tens of electron skin depths. For electron-positron plasmas, we find generation of alternating currents and magnetic fields. Jet and sheath plasmas are accelerated across the shear surface in the strong magnetic fields generated by the kKHI. The mixing of jet and sheath plasmas generates a transverse structure similar to that produced by the Weibel instability.

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Author details:Ken-Ichi Nishikawa, P. E. Hardee, I. Dutan, J. Niemiec, M. Medvedev, Y. Mizuno, A. Meli, H. Sol, B. Zhang, Martin PohlORCiDGND, D. H. Hartmann
DOI:https://doi.org/10.1088/0004-637X/793/1/60
ISSN:0004-637X
ISSN:1538-4357
Title of parent work (English):The astrophysical journal : an international review of spectroscopy and astronomical physics
Publisher:IOP Publ. Ltd.
Place of publishing:Bristol
Publication type:Article
Language:English
Year of first publication:2014
Publication year:2014
Release date:2017/03/27
Tag:acceleration of particles; magnetic fields; plasmas; radiation mechanisms: non-thermal; relativistic processes; stars: jets
Volume:793
Issue:1
Number of pages:16
Funding institution:NSF [AST-0908010, AST-0908040, NASA-NNG05GK73G, NNX07AJ88G, NNX08AG83G, NNX08AL39G, NNX09AD16G, NNX12AH06G, NNX13AP-21G, NNX13AP14G]; Polish National Science Centre [DEC-2011/01/B/ST9/03183, DEC-2012/04/A/ST9/00083]; Ministry of Science and Technology of Taiwan [NSC 100-2112-M-007-022-MY3, MOST 103-2112-M-007-023-MY3]; Deutsche Forschungsgemeinschaft [PO 1508/1-2]; National Science Foundation [PHY05-51164]
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer review:Referiert
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