Weak Electromagnetic Fields Around a Rotating Black Hole

Details Weak Electromagnetic Fields Around a Rotating Black Hole Weak Electromagnetic Fields Around a Rotating Black Hole

May 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvd...5.2455f&link_type=abstract

Physical Review D, vol. 5, Issue 10, pp. 2455-2458

Physics

27

Scientific paper

Foundations are laid for studying weak electromagnetic fields around a rotating black hole. In particular, Maxwell's equations in the Kerr geometry of the black hole are reduced to a single second-order partial differential equation. Although this differential equation is probably not separable, it is sufficiently simple to yield theorems about electromagnetic properties of black holes.

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