Generalization of Kerr spacetime
Hernando QuevedoInstitute for Theoretical Physics, University of Cologne, D-5000 Cologne 41, Federal Republic of GermanyBahram MashhoonInstitute for Theoretical Physics, University of Cologne, D-5000 Cologne 41, Federal Republic of Germany
1991en
ABI
Аннотация
A class of exact solutions of the Einstein-Maxwell equations is presented. It represents the exterior gravitational field of a charged rotating mass. The class contains a generalization of the charged Kerr metric involving an infinite set of parameters that pertain to an axisymmetric deformation of the source.
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