The general Kerr–de Sitter metrics in all dimensions
We give the general Kerr–de Sitter metric in arbitrary space–time dimension D ≥ 4 , with the maximal number [ ( D − 1 ) / 2 ] of independent rotation parameters. We obtain the metric in Kerr–Schild form, where it is written as the sum of a de Sitter metric plus the square of a null-geodesic vector,...
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Published in | Journal of geometry and physics Vol. 53; no. 1; pp. 49 - 73 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
2005
|
Subjects | |
Online Access | Get full text |
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Summary: | We give the general Kerr–de Sitter metric in arbitrary space–time dimension
D
≥
4
, with the maximal number
[
(
D
−
1
)
/
2
]
of independent rotation parameters. We obtain the metric in Kerr–Schild form, where it is written as the sum of a de Sitter metric plus the square of a null-geodesic vector, and in generalised Boyer–Lindquist coordinates. The Kerr–Schild form is simpler for verifying that the Einstein equations are satisfied, and we have explicitly checked our results for all dimensions
D
≤
11
. We discuss the global structure of the metrics, and obtain formulae for the surface gravities and areas of the event horizons. We also obtain the Euclidean-signature solutions, and we construct complete non-singular compact Einstein spaces on associated
S
D
−
2
bundles over
S
2
, infinitely many for each odd
D
≥
5
. |
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ISSN: | 0393-0440 1879-1662 |
DOI: | 10.1016/j.geomphys.2004.05.001 |