Isolated solitons in an ultrarelativistic electron-positron plasma of a pulsar magnetosphere

Details Isolated solitons in an ultrarelativistic electron-positron plasma of a pulsar magnetosphere Isolated solitons in an ultrarelativistic electron-positron plasma of a pulsar magnetosphere

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrva..40.2203m&link_type=abstract

Physical Review A - General Physics, 3rd Series (ISSN 0556-2791), vol. 40, Aug. 15, 1989, p. 2203-2206.

Statistics

Computation

19

Computational Astrophysics, Electron Plasma, Pulsar Magnetospheres, Relativistic Plasmas, Solitary Waves, Einstein Equations, Maxwell Equation, Ponderomotive Forces, Space-Time Functions, Stellar Models

Scientific paper

An earlier investigation of the nonlinear propagation of intense electromagnetic radiation in a pulsar magnetosphere is extended here to include ultrarelativistic effects. The macroscopic behavior of an ultrarelativistic plasma is considered in a covariant form. Relativistic and time-derivative ponderomotive nonlinearities are accounted for. Weak relativistic effects are found to excite the envelope solitons, while the ultrarelativistic nonlinearity generates isolated solitons in the plasma, so that the electric or magnetic fields appear as isolated spikes.

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