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 (2)

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

Cited by in corpus (4)

• Higher-Dimensional Black Holes: Hidden Symmetries and Separation of Variables
• On conformal Killing-Yano tensors for Plebanski-Demianski family of solutions
• Electromagnetic Field in Higher-Dimensional Black-Hole Spacetimes
• Rotating Spacetimes with Asymptotic Non-Flat Structure and the Gyromagnetic Ratio