Uniqueness of Kerr-Newman solution
General Relativity and Quantum Cosmology
2014-07-22 v1
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.
Keywords
Cite
@article{arxiv.1407.5381,
title = {Uniqueness of Kerr-Newman solution},
author = {A. K. M. Masood-ul-Alam},
journal= {arXiv preprint arXiv:1407.5381},
year = {2014}
}