Hidden Symmetries and Geodesics of Kerr spacetime in Kaluza-Klein Theory
Alikram N. Aliev, Goksel Daylan Esmer

TL;DR
This paper investigates the hidden symmetries and geodesic properties of Kerr black holes in Kaluza-Klein theory, revealing how extra dimensions influence orbital stability and the structure of spacetime.
Contribution
It demonstrates the separability of the Hamilton-Jacobi equation for massless geodesics and constructs explicit conformal Killing tensors in Kerr-Kaluza-Klein spacetime.
Findings
Complete separation occurs only for massless geodesics.
Extra dimension enlarges regions of stable and bounded orbits.
Analytical formulas for orbital frequencies and stability boundaries.
Abstract
The Kerr spacetime in Kaluza-Klein theory describes a rotating black hole in four dimensions from the Kaluza-Klein point of view and involves the signature of an extra dimension that shows up through the appearance of the electric and dilaton charges. In this paper, we study the separability properties of the Hamilton-Jacobi equation for geodesics and the associated hidden symmetries in the spacetime of the Kerr-Kaluza-Klein black hole. We show that the complete separation of variables occurs only for massless geodesics, implying the existence of hidden symmetries generated by a second rank conformal Killing tensor. Employing a simple procedure built up on an "effective" metric, which is conformally related to the original spacetime metric and admits a complete separability structure, we construct the explicit expression for the conformal Killing tensor. Next, we study the properties of…
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