arXiv · hep-th/0309227
On quasi-normal modes of Kerr black holes
Abstract
We calculate analytically asymptotic values of quasi-normal frequencies of four-dimensional Kerr black holes by solving the Teukolsky wave equation. We obtain an expression for arbitrary spin of the wave in agreement with Hod's proposal which is based on Bohr's correspondence principle. However, the range of frequencies is bounded from above by $1/a$, where $a$ is the angular momentum per unit mass of the black hole. Our argument is only valid in the small-$a$ limit which includes the Schwarzschild case.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Suphot Musiri, George Siopsis. 2003-09-24. On quasi-normal modes of Kerr black holes. https://doi.org/10.1016/j.physletb.2003.10.109
Cite the original work for its findings. Save a collection to share your selection of sources.