Volume 429, Number 3, January III 2005
|Page(s)||779 - 784|
|Published online||05 January 2005|
A stability property of a force-free surface bounding a vacuum gap
CEA/DSM/DAPNIA, Service d'Astrophysique (CNRS FRE 2591), CE Saclay, 91191 Gif-sur-Yvette Cedex, France e-mail: firstname.lastname@example.org
Accepted: 8 September 2004
A force-free surface (FFS) is a sharp boundary separating a void from a region occupied by a charge-separated force-free plasma. It is proven here under very general assumptions that there is on a simple relation between the charge density μ on the plasma side and the derivative of along on the vacuum side (with denoting the electric field and the magnetic field). Combined with the condition on , this relation implies that a FFS has a general stability property, already conjectured by Michel (1979, ApJ 227, 579): turns out to attract charges placed on the vacuum side if they are of the same sign as μ. In the particular case of a FFS existing in the axisymmetric stationary magnetosphere of a “pulsar”, the relation is given a most convenient form by using magnetic coordinates, and is shown to imply an interesting property of a gap. Also, a simple proof is given of the impossibility of a vacuum gap forming in a field which is either uniform or radial (monopolar).
Key words: stars: pulsars: general / magnetic fields / plasmas
© ESO, 2005
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