Quantization of horizon area of Kerr-Newman-de Sitter black hole
arXiv:1902.01705 · doi:10.1088/0256-307X/36/3/030401
Abstract
Using the adiabatic invariant action and applying Bohr-Sommerfeld quantization rule and first law of black hole thermodynamics a study of quantization of entropy and horizon area of Kerr-Newman-de Sitter black hole is carried out. The same entropy spectrum is obtained in two different coordinate systems. It is also observed that the spacing of the entropy spectrum is independent of the black hole parameters and also the corresponding quantum of horizon area is in agreement with the results of Bekenstein.
Accepted in Chinese Physics Letters
References in corpus (6)
- The physical interpretation of the spectrum of black hole quasinormal modes
- Area spectrum of rotating black holes via the new interpretation of quasinormal modes
- Quantization of the black hole area as quantization of the angular momentum component
- Spectroscopy of a Reissner-Nordström black hole via an action variable
- Periodicity and area spectrum of black holes
- Role of Horizons in Semiclassical Gravity: Entropy and the Area Spectrum