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A&A 366, 129-137 (2001)
DOI: 10.1051/0004-6361:20000031
Pulsar magnetospheres: Numerical simulations of large amplitude electron-positron oscillations
A. A. da Costa1, 2, D. A. Diver1 and G. A. Stewart11 Dept. of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, Scotland, UK
2 Centro de Electrodinâmica, Instituto Superior Técnico, 1049-001 Lisboa, Portugal
(Received 21 September 2000 / Accepted 24 October 2000 )
Abstract
The numerical simulation of non-linear electron-positron oscillations is reported, showing the evolution of the electric field
and the plasma number density for large amplitude disturbances. Sharp density gradients and changes in the oscillation frequency
are demonstrated, and a new analytical framework is presented to illustrate these phenomena, particularly in the context of
pulsar plasmas.
Key words: pulsars: general -- plasmas
Offprint request: D. A. Diver, diver@astro.gla.ac.uk
© ESO 2001
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