arXiv · 2607.16581
Separating the linearized Einstein equations in Kerr
Abstract
A direct separation of the linearized Einstein equations in Kerr is presented. The trace of the perturbed metric is found to obey the spin-0 perturbation equation and so is irrelevant for the spin-2 perturbations. By combining the traceless condition, the Killing-Yano symmetry, a parity requirement, and the de Donder gauge condition, it has been found possible to reduce the linearized Einstein equations in Kerr to a manageable level, thereby enabling the direct separation of the equations and the derivation of a unique set of decoupled mode functions for the spin-2 perturbation of the Kerr black hole.
Explore related subjects
Keep this discovery
Jianwei Mei. 2026-07-18. Separating the linearized Einstein equations in Kerr. https://arxiv.org/abs/2607.16581
Cite the original work for its findings. Save a collection to share your selection of sources.