arXiv · 0811.3794
On Uniqueness of Kerr Space-time near null infinity
Abstract
We re-express the Kerr metric in standard Bondi-Saches' coordinate near null infinity ${\cal I}^+$. Using the uniqueness result of characteristic initial value problem, we prove the Kerr metric is the only asymptotic flat, stationary, axial symmetric, Type-D solution of vacuum Einstein equation. The Taylor series of Kerr space-time is expressed in terms of B-S coordinates and the N-P constants have been calculated.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Xiaoning Wu, Shan Bai. 2008-11-24. On Uniqueness of Kerr Space-time near null infinity. https://doi.org/10.1103/physrevd.78.124009
Cite the original work for its findings. Save a collection to share your selection of sources.