On Kerr black hole deformations admitting a Carter constant and an invariant criterion for the separability of the wave equation

DOI10.1007/s10714-021-02795-2zbMath1476.83003arXiv2007.12125OpenAlexW3131553857MaRDI QIDQ2060473

Kostas D. Kokkotas, Georgios Papadopoulos

Publication date: 13 December 2021

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2007.12125

zbMATH Keywords

Klein-Gordon equationseparabilityintegrals of motionKilling tensorsCarter constantKerr deformations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (3)

The eye of the storm: a regular Kerr black hole ⋮ Constant-\(r\) geodesics in the Painlevé-Gullstrand form of Lense-Thirring spacetime ⋮ Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics

Cites Work

• Unnamed Item
• Preserving Kerr symmetries in deformed spacetimes
• Rotating charged black hole solution in heterotic string theory
• Mapping spacetimes with LISA: inspiral of a test body in a ‘quasi-Kerr’ field
• Global Structure of the Kerr Family of Gravitational Fields

This page was built for publication: On Kerr black hole deformations admitting a Carter constant and an invariant criterion for the separability of the wave equation