On the parameters of the Kerr-NUT-(anti-)de Sitter space-time
arXiv:gr-qc/0702042 · doi:10.1088/0264-9381/24/6/N02
Abstract
Different forms of the metric for the Kerr-NUT-(anti-)de Sitter space-time are being widely used in its extension to higher dimensions. The purpose of this note is to relate the parameters that are being used to the physical parameters (mass, rotation, NUT and cosmological constant) in the basic four dimensional situation.
arXiv comment4 pages. To appear as a Note in Classical and Quantum Gravity
References in corpus (8)
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- General Kerr-NUT-AdS Metrics in All Dimensions
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- Charged Vector Particles Tunneling From A Pair of Accelerating and Rotating and Gauged Super-Gravity Black Holes
- Tunneling of Massive Vector Particles under the Influence of Quantum Gravity
- Fermions Tunneling from Charged Accelerating and Rotating Black Holes with NUT Parameter
- Isomonodromy, Painlevé Transcendents and Scattering off of Black Holes
- Electromagnetic Field in Higher-Dimensional Black-Hole Spacetimes
- Identification of black hole horizons using scalar curvature invariants
- Rotating Spacetimes with Asymptotic Non-Flat Structure and the Gyromagnetic Ratio
- Fermionic and Bosonic Greybody Factors as well as Quasinormal Modes for Charged Taub NUT Black Holes
- Greybody Radiation of scalar and Dirac perturbations of NUT Black Holes
- On hidden symmetries of extremal Kerr-NUT-AdS-dS black holes
- General Wahlquist Metrics in All Dimensions
- Curvature invariant characterization of event horizons of four-dimensional black holes conformal to stationary black holes
- Hawking radiation of scalars from charged accelerating and rotating black holes with NUT parameter
- NUT-like and near-horizon limits of Kerr-NUT-(A)dS spacetimes
- Non-singular extension of the Kerr-NUT-(anti) de Sitter spacetimes
- Projectively non-singular horizons in Kerr-NUT-de Sitter spacetimes
- On local equivalence problem of spacetimes with two orthogonally transitive commuting Killing fields
- Effect of NUT parameter on the analytic extension of the Cauchy horizon that develop in colliding wave spacetimes