Abstract
Pseudostationary asymptotically flat axisymmetric black-hole solutions of the source-free Einstein-Maxwell equations are considered. It is shown that these solutions form discrete continuous families, each depending on at most four parameters, of which only one—the Kerr-Newman family—contains members with zero angular momentum.
- Received 20 August 1973
DOI:https://doi.org/10.1103/PhysRevD.10.458
©1974 American Physical Society
