Phys. Rev. Lett. 96, 105002 (2006) [4 pages]
Space-Charge Effects in the Current-Filamentation or Weibel Instability
Abstract
References (14)
Citing Articles
M. Tzoufras, 1 C. Ren, 2 F. S. Tsung, 3 J. W. Tonge, 3 W. B. Mori, 1,3 M. Fiore, 4 R. A. Fonseca, 4 and L. O. Silva41Department of Electrical Engineering, University of California, Los Angeles, California 90095, USA
2Departments of Mechanical Engineering and Physics and Astronomy, University of Rochester, Rochester, New York 14623, USA and Laboratory for Laser Energetics, University of Rochester, Rochester, New York 14623, USA
3Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA
4GoLP/Centro de Fisica dos Plasmas, Instituto Superior Tecnico, 1049-001 Lisboa, Portugal
Received 13 October 2005; published 15 March 2006
We consider how an unmagnetized plasma responds to an incoming flux of energetic electrons. We assume a return current is present and allow for the incoming electrons to have a different transverse temperature than the return current. To analyze this configuration we present a nonrelativistic theory of the current-filamentation or Weibel instability for rigorously current-neutral and nonseparable distribution functions, f0(px,py,pz) fx(px)fy(py)fz(pz). We find that such distribution functions lead to lower growth rates because of space-charge forces that arise when the forward-going electrons pinch to a lesser degree than the colder, backward-flowing electrons. We verify the growth rate, range of unstable wave numbers, and the formation of the density filaments using particle-in-cell simulations.
©2006 The American Physical Society
REFERENCES (14)
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