A boundary value problem for the five-dimensional stationary rotating black holes

Preprint

24 January 2004

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/0401100

Abstract

We study the boundary value problem for the stationary rotating black hole solutions to the five-dimensional vacuum Einstein equation. Assuming the two commuting rotational symmetry and the sphericity of the horizon topology, we show that the black hole is uniquely characterized by the mass, and a pair of the angular momenta.

Keywords

DIMENSIONAL STATIONARY
BOUNDARY VALUE PROBLEM
STATIONARY ROTATING
EINSTEIN EQUATION
ROTATING BLACK
BLACK HOLE
COMMUTING
VACUUM

All Related Versions

Version 1, 2004-01-24, ArXiv
Published version: Physical Review D, 69 (12), 124005.

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