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Electron Acceleration by Strong DC Electric Fields in Extragalactic Jets

Published online by Cambridge University Press:  25 May 2016

Y. E. Litvinenko
Y. E. Litvinenko*
Affiliation:
Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824-3525, U.S.A.

Abstract

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Fast magnetic reconnection in extragalactic jets leads to electron acceleration by the DC electric field in the reconnecting current sheet. The maximum electron energy (γ > 106) and the acceleration time (< 106 s) are determined by the magnetic field dynamics in the sheet.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 311 - 312
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Eilek, J. A., & Hughes, P. A. 1991, in Beams and Jets in Astrophysics, ed. Hughes, P. A. (Cambridge: Cambridge Univ. Press), 428.Google Scholar
Hill, T. W. 1975, J. Geophys. Res., 80, 4689.CrossRefGoogle Scholar
Litvinenko, Y. E. 1996, ApJ, 462, 997.Google Scholar
Litvinenko, Y. E. 1999, A&A, 349, 685.Google Scholar