Abstract
AbstractWe uncover hidden spectral symmetries of the Teukolsky equation in Kerr(-de Sitter) black holes, recently conjectured by Aminov, Grassi and Hatsuda (Ann. Henri Poincaré 23, 1951-1977, 2022, and Gen. Relativ. Grav. 53(10):93, 2021) in the zero cosmological constant case. Using these symmetries, we provide a new, simpler proof of mode stability for subextremal Kerr black holes. We also present a partial mode stability result for Kerr–de Sitter black holes.
Funder
engineering and physical sciences research council
conselho nacional de desenvolvimento científico e tecnológico
Directorate for Mathematical and Physical Sciences
Publisher
Springer Science and Business Media LLC
Subject
Mathematical Physics,Statistical and Nonlinear Physics
Reference63 articles.
1. Aminov, G., Grassi, A., Hatsuda, Y.: Black Hole Quasinormal Modes and Seiberg-Witten Theory. Ann. Henri Poincaré 23, 1951–1977 (2022)
2. Andersson, L., Ma, S., Paganini, C., Whiting, B.F.: Mode stability on the real axis. J. Math. Phys. 58(7), 072501 (2017)
3. Bianchi, M., Consoli, D., Grillo, A., Morales, J. F.: QNMs of branes, BHs and fuzzballs from Quantum SW geometries. Preprint (2021) arXiv:2105.04245
4. Bonelli, G., Iossa, C., Lichtig, D. P., Tanzini, A.: Exact solution of Kerr black hole perturbations via CFT$$_2$$ and instanton counting. Preprint (2021) arXiv:2105.04483
5. Boyer, R.H., Lindquist, R.W.: Maximal Analytic Extension of the Kerr Metric. J. Math. Phys. 8(2), 265–281 (1967)
Cited by
7 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献