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Astron. Astrophys. 327, 662-670

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Acceleration of relativistic plasma in the magnetosphere
of an axisymmetric rotator

S.V. Bogovalov

Moscow Engineering Physics Institute, Kashirskoje Shosse 31, 115409 Moscow, Russia (e-mail: bogoval@photon.mephi.ru)

Received 6 November 1996 / Accepted 11 June 1997


The flow of relativistic plasma in the magnetosphere of an axisymmetrical rotator is considered analytically as well as numerically. The selfconsistent solution of the plasma outflow in a monopole-like poloidal magnetic field is obtained accurately up to terms proportional to FORMULA, where FORMULA is Michel's magnetization parameter, FORMULA, while FORMULA and v0 are the initial Lorentz-factor and the velocity of the plasma. It is shown that under the condition FORMULA typical for real radio pulsars, the plasma is not accelerated and is not collimated in the subsonic region. Numerical simulation of the time dependent version of this problem shows that the stationary flow of relativistic plasma is apparently unstable when FORMULA. This instability of the flow leads to the acceleration of the plasma.

Key words: MHD - pulsars; jets and outflows - galaxies; jets

© European Southern Observatory (ESO) 1997

Online publication: October 14, 1997
Last change: April 6, 1998