Area spectrum of slowly rotating black holes
arXiv:1003.3519 · doi:10.1016/j.physletb.2010.04.041
Abstract
We investigate the area spectrum for rotating black holes which are Kerr and BTZ black holes. For slowly rotating black holes, we use the Maggiore's idea combined with Kunstatter's method to derive their area spectra, which are equally spaced.
5 pages, v2: some points clarified and references added
References in corpus (9)
- The physical interpretation of the spectrum of black hole quasinormal modes
- Area spectrum of rotating black holes via the new interpretation of quasinormal modes
- Quantum tunneling and black hole spectroscopy
- On the Kerr Quantum Area Spectrum
- Spinning Dilaton Black Holes in 2 +1 Dimensions: Quasi-normal Modes and the Area Spectrum
- Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
- Analytic Study of Rotating Black-Hole Quasinormal Modes
- Asymptotic Spectroscopy of Rotating Black Holes
- Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime
Cited by in corpus (14)
- Stability Analysis and Area Spectrum of 3-Dimensional Lifshitz Black Holes
- On black hole spectroscopy via adiabatic invariance
- Slowly rotating black holes in the Horava-Lifshitz gravity
- Area spectrum of the d-dimensional Reissner-Nordstrom black hole in the small charge limit
- Spectroscopy of Rotating Linear Dilaton Black Holes From Boxed Quasinormal Modes
- Entropy spectra of black holes from resonance modes in scattering by the black holes
- Entropy spectrum of a Kerr anti-de Sitter black hole
- Entropy spectrum of the D-dimensional massless topological black hole
- Quantization of horizon area of Kerr-Newman-de Sitter black hole
- Entropy spectra of single horizon black holes in two dimensions
- Gravitational surface Hamiltonian and entropy quantization
- Area spectrum of Schwarzschild black hole inspired by noncommutative geometry
- Scalar Clouds and Quasinormal Modes
- On black hole spectroscopy via quantum tunneling