Area spectrum of the D-dimensional de Sitter spacetime
arXiv:0910.5779 · doi:10.1016/j.physletb.2009.10.091
Abstract
The determination of the quantum area spectrum of a black hole horizon by means of its asymptotic quasinormal frequencies has been explored recently. We believe that for D-dimensional de Sitter horizon we must study if the idea works. Thus taking into account the local description of the thermodynamics of horizons proposed by Padmanabhan and the results of Hod, Kunstatter, and Maggiore we study the area spectrum of the D-dimensional de Sitter horizon.
6 pages, accepted for publication in Physics Letters B
References in corpus (15)
- The physical interpretation of the spectrum of black hole quasinormal modes
- Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
- Area spectrum of rotating black holes via the new interpretation of quasinormal modes
- Is gravitational entropy quantized ?
- Quasinormal modes of D-dimensional de Sitter spacetime
- On the Kerr Quantum Area Spectrum
- Spinning Dilaton Black Holes in 2 +1 Dimensions: Quasi-normal Modes and the Area Spectrum
- Quantization of the black hole area as quantization of the angular momentum component
- Dirac quasinormal modes of D-dimensional de Sitter spacetime
- Area spectrum of near-extremal SdS black holes via the new interpretation of quasinormal modes
- Quantization of Black Hole Entropy from Quasinormal Modes
- Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime
- On the "Universal" Quantum Area Spectrum
- Role of Horizons in Semiclassical Gravity: Entropy and the Area Spectrum
- A brief commentary on black hole entropy