Kerr–de Sitter black holes with NUT charges

@article{Chen2007KerrdeSB,
  title={Kerr–de Sitter black holes with NUT charges},
  author={W. Y. Chen and H. Q. Lu and C N Pope},
  journal={Nuclear Physics},
  year={2007},
  volume={762},
  pages={38-54}
}
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62 Citations
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2
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26
Methods Citations
12
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1

62 Citations

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Construction of Einstein-Sasaki metrics in D≥7
We construct explicit Einstein-Kaehler metrics in all even dimensions D=2n+4{>=}6, in terms of a 2n-dimensional Einstein-Kaehler base metric. These are cohomogeneity 2 metrics which have the new…
A pr 2 00 8 MIFP-08-06 New Black Holes in Five Dimensions
We construct new stationary Ricci-flat metrics of cohomogeneity 2 in five dimensions, which generalise the Myers-Perry rotating black hole metrics by adding a further non-trivial parameter. We obtain…
A Killing tensor for higher dimensional Kerr-AdS black holes with NUT charge
In this paper, we study the recently discovered family of higher dimensional Kerr-AdS black holes with an extra NUT-like parameter. We show that the inverse metric is additively separable after…
On Hidden Symmetries of d>4 NHEK-N-AdS Geometry
As well known, all higher dimensional Kerr-NUT-Ads metrics with arbitrary rotation and NUT parameters in an asymptotically AdS spacetime have a new hidden symmetry. In this paper, we show that in the…
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References

SHOWING 1-10 OF 20 REFERENCES
Separability and Killing tensors in Kerr–Taub-NUT–de Sitter metrics in higher dimensions
The General Kerr-de Sitter metrics in all dimensions
Construction of Einstein-Sasaki metrics in D≥7
We construct explicit Einstein-Kaehler metrics in all even dimensions D=2n+4{>=}6, in terms of a 2n-dimensional Einstein-Kaehler base metric. These are cohomogeneity 2 metrics which have the new…
Rotating black holes in gauged supergravities: Thermodynamics, supersymmetric limits, topological solitons and time machines
We study the thermodynamics of the recently-discovered non-extremal charged rotating black holes of gauged supergravities in five, seven and four dimensions, obtaining energies, angular momenta and…
Anti-de Sitter-space/conformal-field-theory Casimir energy for rotating black holes.
TLDR
It is shown that, if one chooses the Einstein static universe as the metric on the conformal boundary of Kerr-anti-de Sitter spacetime, then the Casimir energy of the boundary conformal field theory can easily be determined and straightforwardly obeys the first law of thermodynamics.
New Einstein-Sasaki and Einstein Spaces from Kerr-de Sitter
In this paper, which is an elaboration of our results in Phys. Rev. Lett. 95:071101, 2005 (hep-th/0504225), we construct new Einstein-Sasaki spaces Lp,q,r1,...,rn−1 in all odd dimensions D = 2n+1 ≥…
Supersymmetric Kerr-anti-de Sitter solutions
We prove the existence of one quarter supersymmetric type IIB configurations that arise as nontrivial scaling solutions of the standard five-dimensional Kerr-anti-de Sitter black holes by the…
Rotation and the AdS/CFT correspondence
In asymptotically flat space a rotating black hole cannot be in thermodynamic equilibrium because the thermal radiation would have to be co-rotating faster than light far from the black hole. However…
AdS/CFT Casimir Energy for Rotating Black Holes
We show that if one chooses the Einstein Static Universe as the metric on the conformal boundary of Kerr-AdS spacetime, then the Casimir energy of the boundary conformal field theory can easily be…
New Einstein-Sasaki spaces in five and higher dimensions.
We obtain infinite classes of new Einstein-Sasaki metrics on complete and nonsingular manifolds. They arise, after Euclideanization, from BPS limits of the rotating Kerr-de Sitter black hole metrics.…
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