Black-hole magnetostatics

Details Black-hole magnetostatics Black-hole magnetostatics

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mapr...81..149k&link_type=abstract

Mathematical Proceedings, vol. 81, Jan. 1977, p. 149-156. Research supported by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Black Holes (Astronomy), Magnetostatics, Maxwell Equation, Multipolar Fields, Space-Time Functions

Scientific paper

The notions that the black-hole background geometry at a stationary state is a member of the Kerr-Newman family of metrics and any charge on the hole is small enough to be treated as a perturbation on the Kerr black-hole background are briefly discussed, after which the paper presents the stationary non-axisymmetric multipole solutions of the Maxwell equations for the perturbing electromagnetic field on the Kerr background. Appropriate boundary conditions, such as the condition that no physically well-behaved observer sees infinite fields near the hole, are imposed and integrability conditions for those equations are used.

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