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General Relativistic Magnetoionic Theory

Broderick, Avery and Blandford, Roger (2003) General Relativistic Magnetoionic Theory. Astrophysics and Space Science, 288 (1-2). pp. 161-173. ISSN 0004-640X. https://resolver.caltech.edu/CaltechAUTHORS:20190607-154608495

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Abstract

We have developed methods for tracing rays and performing radiative transfer through a magneto active 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1023/B:ASTR.0000005003.18358.b9DOIArticle
https://rdcu.be/bFVW5PublisherFree ReadCube access
ORCID:
AuthorORCID
Broderick, Avery0000-0002-3351-760X
Blandford, Roger0000-0002-1854-5506
Additional Information:© 2003 Kluwer Academic Publishers. The authors would like thank Eric Agol for a number of useful conversations and comments regarding this work. This has been supported by NASA grants 5-2837 and 5-12032.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NASA5-2837
NASA5-12032
Subject Keywords:Black Hole; Circular Polarisation; Ordinary Mode; Magnetoactive Plasma; General Relativistic Effect
Issue or Number:1-2
Record Number:CaltechAUTHORS:20190607-154608495
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190607-154608495
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96218
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:08 Jun 2019 17:58
Last Modified:03 Oct 2019 21:20

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