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

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

2004-01-24

arxiv.org/abs/gr-qc/0401100v1

Phys.Rev.D69:124005,2004

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages, no figures

Scientific paper

10.1103/PhysRevD.69.124005

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.

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