Arbitrarily deformed Kerr-Newman black hole in an external gravitational field

Details Arbitrarily deformed Kerr-Newman black hole in an external gravitational field Arbitrarily deformed Kerr-Newman black hole in an external gravitational field

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvd..57.3382b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 57, Issue 6, 15 March 1998, pp.3382-3388

Physics

7

Exact Solutions, Black Holes

Scientific paper

An exact axisymmetric solution of the Einstein-Maxwell equations possessing two infinite sets of arbitrary real parameters and able to describe a deformed Kerr-Newman black hole in an external gravitational field is presented in a concise analytic form. The validity of Smarr's mass formula is demonstrated for a Kerr-Newman black hole surrounded by an external static gravitational field.

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