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General Relativistic Electrodynamics of the Magnetic Polar Regions of Neutron Stars

Published online by Cambridge University Press:  27 September 2017

A. G. Muslimov  and
A. I. Tsygan
A. G. Muslimov
Affiliation:
A. F. Ioffe Institute of Physics and Technology
A. I. Tsygan
Affiliation:
A. F. Ioffe Institute of Physics and Technology

Abstract

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The induction of the electric fields near a rotating neutron star is considered within the framework of General Relativity. It is demonstrated that within the open magnetic field region, filled by relativistically moving charged particles, a sufficiently strong component of the electric field is generated. This component is due to the effect of dragging of inertial frames of reference and predominates in the case when a neutron star is not exactly an orthogonal rotator. Finally, we discuss some implications of our results on the theory of radio pulsars.

Type
Part VI Polar cap theories
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 248 - 251
Copyright
Copyright © United States Naval Observatory 1992