Published August 1989 | Version v1
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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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MF available from INIS under the Report Number.

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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