Geodesics and Symmetries of Doubly-Spinning Black Rings
arXiv:0812.0235 · doi:10.1088/0264-9381/26/8/085016
Abstract
This paper studies various properties of the Pomeransky-Sen'kov doubly-spinning black ring spacetime. I discuss the structure of the ergoregion, and then go on to demonstrate the separability of the Hamilton-Jacobi equation for null, zero energy geodesics, which exist in the ergoregion. These geodesics are used to construct geometrically motivated coordinates that cover the black hole horizon. Finally, I relate this weak form of separability to the existence of a conformal Killing tensor in a particular 4-dimensional spacetime obtained by Kaluza-Klein reduction, and show that a related conformal Killing-Yano tensor only exists in the singly-spinning case.
Minor corrections/clarifications and references added, results of paper unchanged. Accepted for publication by Class. Quant. Grav. (26 pages, 5 figures)
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Cited by in corpus (8)
- Dynamics of test particles in the general five-dimensional Myers-Perry spacetime
- Geodesic Motion in the Singly Spinning Black Ring Spacetime
- Geodesic Motion in the (Charged) Doubly Spinning Black Ring Spacetime
- Stable Bound Orbits around Black Rings
- Chaos in Geodesic Motion around a Black Ring
- A Charged Doubly Spinning Black Ring
- Algebraic classification of five-dimensional spacetimes using scalar invariants
- Integrability of Particle System around a Ring Source as the Newtonian Limit of a Black Ring