On the parameters of the Kerr-NUT-(anti-)de Sitter space-time

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.

4 pages. To appear as a Note in Classical and Quantum Gravity

References in corpus (3)

• General Kerr-NUT-AdS Metrics in All Dimensions
• Complete Integrability of Geodesic Motion in General Kerr-NUT-AdS Spacetimes
• Hidden Symmetry of Higher Dimensional Kerr-NUT-AdS Spacetimes

Cited by in corpus (11)

• Higher-Dimensional Black Holes: Hidden Symmetries and Separation of Variables
• On conformal Killing-Yano tensors for Plebanski-Demianski family of solutions
• Isomonodromy, Painlevé Transcendents and Scattering off of Black Holes
• Identification of black hole horizons using scalar curvature invariants
• Electromagnetic Field in Higher-Dimensional Black-Hole Spacetimes
• 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
• Curvature invariant characterization of event horizons of four-dimensional black holes conformal to stationary black holes
• Non-singular extension of the Kerr-NUT-(anti) de Sitter spacetimes