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Lookup NU author(s): Professor Ian MossORCiD
The electromagnetic field around a Kerr black hole inside a current loop is sometimes used as the basis of a toy model for discussing the properties of particle orbits near astrophysical black holes. The motivation for the present paper is to correct the published solution to Maxwell's equations with a charged current loop. Dipole approximations and closed-form expressions in the extreme Kerr limit are also presented. Using the corrected solution, it turns out that imposing a vanishing electromotive force produces a loop with a potential which is finite everywhere outside the black hole. Ring solutions can be combined into solutions with multiple rings or current discs.
Author(s): Moss IG
Publication type: Article
Publication status: Published
Journal: Physical Review D
Year: 2011
Volume: 83
Issue: 12
Print publication date: 27/06/2011
Date deposited: 21/02/2012
ISSN (print): 1550-7998
ISSN (electronic): 1089-4918
Publisher: American Physical Society
URL: http://dx.doi.org/10.1103/PhysRevD.83.124046
DOI: 10.1103/PhysRevD.83.124046
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