Area spectrum and thermodynamics of KS black holes in Hořava gravity
arXiv:1307.6438 · doi:10.1007/s10714-013-1565-2
Abstract
We investigate the area spectrum of Kehagias-Sfetsos black hole in Hořava-Lifshitz gravity via modified adiabatic invariant and Bohr-Sommerfeld quantization rule. We find that the area spectrum is equally spaced with a spacing of . We have also studied the thermodynamic behavior of KS black hole by deriving different thermodynamic quantities.
9 pages, 3 figures. Gen Relativ Gravit 2013
References in corpus (15)
- Quantum Gravity at a Lifshitz Point
- Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
- Membranes at Quantum Criticality
- Horava-Lifshitz Cosmology
- The physical interpretation of the spectrum of black hole quasinormal modes
- Solutions to Horava Gravity
- Cosmology of the Lifshitz universe
- The Black Hole and Cosmological Solutions in IR modified Horava Gravity
- Area spectrum of rotating black holes via the new interpretation of quasinormal modes
- On the Kerr Quantum Area Spectrum
- Black hole spectroscopy via adiabatic invariance
- On black hole spectroscopy via adiabatic invariance
- Spacing of the entropy spectrum for KS Black hole in Horava-Lifshitz gravity
- Discussion on Event Horizon and Quantum Ergosphere of Evaporating Black Holes in a Tunnelling Framework
- Local thermodynamics of KS black hole
Cited by in corpus (4)
- Thermodynamics and Thermodynamic geometry of Park black hole
- A unified thermodynamic picture of Hořava-Lifshitz black hole in arbitrary space time
- Entropy spectrum of the apparent horizon of Vaidya black holes via adiabatic invariance
- Thermodynamics and Quasinormal modes of Park black hole in Hořava gravity