Abstract
It is shown that large-amplitude stationary solitary electrostatic waves can exist in a symmetric plasma (e − e + or C −60 C +60 ), and the relevant parameter ranges (i.e., the range of the Mach numbers and the degree to which the plasma should be nonequilibrium) are determined. The basic requirement for the existence of such waves, specifically, that the symmetric plasma be in a nonequilibrium state, can easily be satisfied in low-density collisionless ideal plasmas under laboratory conditions.
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References
S. L. Shapiro and S. A. Teukolsky, Black Holes, White Dwarfs, and Neutron Stars: the Physics of Compact Objects (Wiley, New York, 1983; Mir, Moscow, 1985).
R. G. Greaves and C. M. Surko, Phys. Rev. Lett. 75, 3846 (1995).
C. M. Surko and R. G. Greaves, Phys. Plasmas 11, 2333 (2004).
H. Boehmer, M. Adams, and N. Rynn, Phys. Plasmas 2, 4369 (1995).
E. P. Liang, S. C. Wilks, and M. Tabak, Phys. Rev. Lett. 81, 4887 (1998).
W. Oohara and R. Hatakeyama, Phys. Rev. Lett. 91, 205005 (2003).
F. Verheest, Nonlin. Processes Geophys. 12, 569 (2005).
R. Z. Sagdeev, in Reviews of Plasma Physics, Ed. by M. A. Leontovich (Atomizdat, Moscow, 1964; Consultants Bureau, New York, 1968), Vol. 4.
A. E. Dubinov, I. D. Dubinova, and S. A. Saĭkov, Lambert W Function: Table of Integrals and Other Mathematical Properties (SarFTI, Sarov, 2004) [in Russian].
S. R. Valluri, D. J. Jeffrey, and R. M. Corless, Can. J. Phys. 78, 823 (2000).
I. D. Dubinova, Fiz. Plazmy 30, 937 (2004) [Plasma Phys. Rep. 30, 872 (2004)].
A. A. Vedenov, E. P. Velikhov, and R. Z. Sagdeev, Yad. Sintez 1, 82 (1961).
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Original Russian Text © V.A. Gordienko, I.D. Dubinova, A.E. Dubinov, 2006, published in Fizika Plazmy, 2006, Vol. 32, No. 11, pp. 987–993.
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Gordienko, V.A., Dubinova, I.D. & Dubinov, A.E. Nonlinear theory of large-amplitude stationary solitary waves in symmetric unmagnetized e − e + and C −60 C +60 plasmas. Plasma Phys. Rep. 32, 910–915 (2006). https://doi.org/10.1134/S1063780X06110043
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DOI: https://doi.org/10.1134/S1063780X06110043