Recovery of black hole mass from a single quasinormal mode
arXiv:2203.13749 · doi:10.1007/s00220-023-04666-0
Abstract
We study the determination of the mass of a de Sitter-Schwarzschild black hole from one quasinormal mode. We prove a local uniqueness result with a Hölder type stability estimate.
References in corpus (5)
- Quasinormal modes of black holes and black branes
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Testing the no-hair theorem with GW150914
- Asymptotic distribution of quasi-normal modes for Kerr-de Sitter black holes
- Quasinormal modes of small Schwarzschild-de Sitter black holes