Hostname: page-component-8448b6f56d-xtgtn Total loading time: 0 Render date: 2024-04-19T22:43:46.156Z Has data issue: false hasContentIssue false

Electro-magnetic fields around a drifting Kerr black hole

Published online by Cambridge University Press:  01 November 2008

Ondřej Kopáček
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic email: kopacek@ig.cas.cz, vladimir.karas@cuni.cz
Vladimír Karas
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic email: kopacek@ig.cas.cz, vladimir.karas@cuni.cz
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A test field solution is constructed, describing the electromagnetic field around a Kerr black hole which is drifting in an arbitrary direction. An asymptotically uniform magnetic field is assumed with a general orientation (with respect to the rotation axis). Lines of force of electric and magnetic intensities are explored, as measured by an observer orbiting around the black hole (above the innermost stable circular orbit, ISCO) or freely falling (below the ISCO) down to the horizon. Magnetic null point is found.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Wald, R. M. 1974, Phys. Rev. D 10, 1680CrossRefGoogle Scholar
Bičák, J. & Janiš, V. 1985, MNRAS 212, 899Google Scholar
Hanni, R. S. & Ruffini, R. 1973, Phys. Rev. D 8, 3259Google Scholar
Jackson, J. D. 1998, Classical electrodynamics, 3rd ed, John Wiley & SonsGoogle Scholar
Bardeen, J. M., Press, W. H., & Teukolsky, S. A. 1972, ApJ 178, 347CrossRefGoogle Scholar
Karas, V. & Kopáček, O. 2008, CQG, in press (arXiv:0811.1772)Google Scholar