General Relativistic Magnetoionic Theory

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To appear in the proceedings of the Amsterdam Circular Polarisation workshop

Scientific paper

10.1023/B:ASTR.0000005003.18358.

We have developed methods for tracing rays and performing radiative transfer through a magnetoactive plasma in a general relativistic environment. The two electromagnetic plasma modes propagate differently due to a combination of dispersive and gravitational effects. We have found that, when given an appropriate environment surrounding the central black hole, it is indeed possible to generate a significant degree of circular polarisation without an appreciable amount of linear polarisation due to these effects alone.

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