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

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.

Authors
Breton N. , Garcia A.A. , Manko V.S. , Denisova T.E.
Number of issue
6
Language
English
Pages
3382-3388
Status
Published
Volume
57
Year
1998
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