Relativistic Langmuir soliton in the magnetosphere of pulsars

Details Relativistic Langmuir soliton in the magnetosphere of pulsars Relativistic Langmuir soliton in the magnetosphere of pulsars

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16..161m&link_type=abstract

(Astrofizika, vol. 16, Jan.-Mar. 1980, p. 161-167.) Astrophysics, vol. 16, no. 1, July 1980, p. 104-108. Translation.

Astronomy and Astrophysics

Astrophysics

9

Plasma Waves, Pulsar Magnetospheres, Pulsars, Relativistic Plasmas, Solitary Waves, Stellar Atmospheres, Astronomical Models, Electron Plasma, Electrostatic Waves, Landau Damping, Maxwell Equation, Nonlinear Equations, Phase Velocity, Schroedinger Equation

Scientific paper

A study is made of the modulation instability of one-dimensional Langmuir waves with phase velocity close to the velocity of light propagating in a relativistic plasma. For these waves, a relativistic kinetic equation and Maxwell's equations are used to obtain a nonlinear Schroedinger equation with allowance for nonlinear Landau damping. The ranges of variation of the plasma parameters for which a relativistic Langmuir soliton can exist are found. Both three- and one-dimensional models of a plasma are considered. It is assumed that the considered processes can take place in the magnetosphere of pulsars.

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