Uniqueness of Kerr-Newman solution

Abstract

We show that non-degenerate multiple black hole solution of Einstein- Maxwell equations in an asymptotically flat axisymmetric spacetime cannot be in stationary equilibrium. This extends the uniqueness of Kerr-Newman solution first proved by Bunting and Mazur in a much wider desirable class. Spin-spin interaction cannot hold the black hole aparts even with electromagnetic forces.

References in corpus (1)

• Non-existence of multiple-black-hole solutions close to Kerr-Newman