Published August 1989
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Ultrarelativistic envelope solitons in electron-positron plasma of the pulsar magnetosphere
Description
The non-linear propagation of intense electromagnetic radiation in pulsar magnetosphere is investigated. The radiation is considered to be a circularly polarized electromagnetic wave, in whose field electron and positron acquire ultrarelativistic velocities. The non-linear frequency shift due to the wave plasma interaction is found to cause the wave localization and it produces a new kind of envelope soliton, which in coupling with the ambient magnetic field generates intense ambipolar field along the magnetic lines. (author). 9 refs
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Additional details
Publishing Information
- Imprint Pagination
- 11 p.
- Report number
- IC--89/176
INIS
- Country of Publication
- International Atomic Energy Agency (IAEA)
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 21016779
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELECTROMAGNETIC RADIATION; ELECTRONS; POSITRONS; PULSARS; RELATIVISTIC PLASMA; SOLITONS; STELLAR MAGNETOSPHERES; WAVE PROPAGATION
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; ATMOSPHERES; COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MATTER; PLASMA; QUASI PARTICLES; RADIATIONS; STELLAR ATMOSPHERES