EFFECTIVE TEMPERATURE, HAWKING RADIATION AND QUASINORMAL MODES
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Publication:4919717
DOI10.1142/S0218271812420230zbMath1266.83105arXiv1205.5251OpenAlexW1980381159MaRDI QIDQ4919717
Publication date: 15 May 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1205.5251
Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Classical and relativistic thermodynamics (80A10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
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Cites Work
- Particle creation by black holes
- A secret tunnel through the horizon
- Gravitation, the quantum and Bohr's correspondence principle.
- Physical Interpretation of the Spectrum of Black Hole Quasinormal Modes
- DO SUBLEADING CORRECTIONS TO BEKENSTEIN–HAWKING ENTROPY HOLD THE KEY TO QUANTUM GRAVITY?
- Spectrum of charged black holes—the big fix mechanism revisited
- Quasi-normal modes: a simple derivation of the level spacing of the frequencies
- Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
- Hawking Radiation As Tunneling
- Black Holes and Entropy
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