Area spectrum and thermodynamics of KS black holes in Hořava gravity
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Publication:376246
DOI10.1007/S10714-013-1565-2zbMath1274.83035arXiv1307.6438OpenAlexW2105114762MaRDI QIDQ376246
V. C. Kuriakose, Jishnu Suresh
Publication date: 4 November 2013
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1307.6438
Black holes (83C57) Geometry and quantization, symplectic methods (81S10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Measures of information, entropy (94A17)
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Cites Work
- Hořava-Lifshitz cosmology
- Evolution of massive fields around a black hole in Hořava gravity
- Gravitation, the quantum and Bohr's correspondence principle.
- Local thermodynamics of KS black hole
- Near extremal Schwarzschild-de Sitter black hole area spectrum from quasi-normal modes
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi></mml:math>-Dimensional Black Hole Entropy Spectrum from Quasinormal Modes
- SPACING OF THE ENTROPY SPECTRUM FOR KS BLACK HOLE IN HOŘAVA–LIFSHITZ GRAVITY
- Physical Interpretation of the Spectrum of Black Hole Quasinormal Modes
- On the Kerr quantum area spectrum
- Non-rotating BTZ black hole area spectrum from quasi-normal modes
- Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
- AREA SPECTRUM OF KERR AND EXTREMAL KERR BLACK HOLES FROM QUASINORMAL MODES
- Hawking Radiation As Tunneling
- Black Holes and Entropy
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