Wave dispersion in gyrotropic relativistic pulsar plasmas

被引:18
|
作者
Luo, Q [1 ]
Melrose, DB [1 ]
Fussell, D [1 ]
机构
[1] Univ Sydney, Sch Phys, Res Ctr Theoret Phys, Sydney, NSW 2006, Australia
来源
PHYSICAL REVIEW E | 2002年 / 66卷 / 02期
关键词
D O I
10.1103/PhysRevE.66.026405
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Wave dispersion in a gyrotropic relativistic pulsar plasma is discussed. A pulsar plasma in general contains electrons, positrons, and possibly ions. Although electron-positron pairs are dominant in number density, charge neutrality is generally not satisfied and the gyrotropic terms need to be considered. These gyrotropic terms can lead to elliptical polarization that may be relevant for the observed circular polarization of pulsar radio emission. The wave dispersion and polarization are obtained numerically by calculating the response in terms of the three relativistic plasma dispersion functions. For waves propagating at an oblique angle (to the ambient magnetic field) a significant ellipticity requires the plasma to deviate substantially from the neutrality condition.
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页数:9
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