Black hole thermodynamics without a black hole?

DOI10.1016/S0550-3213(03)00251-7zbMath1028.83512arXivgr-qc/0302066MaRDI QIDQ1566279

Victor Berezin

Publication date: 1 June 2003

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0302066

zbMATH Keywords

final quantum statequantum gravitational collapsetopological temperature

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45) Quantum equilibrium statistical mechanics (general) (82B10)

Related Items (3)

Zel'dovich states with very small mass and charge in nonlinear electrodynamics coupled to gravity ⋮ Quantum collapse of a self-gravitating thin shell and statistical model of quantum black hole ⋮ CLASSICAL ANALOG OF THE QUANTUM SCHWARZSCHILD BLACK HOLE: LOCAL VS GLOBAL, AND THE MYSTERY OF log 3

Cites Work

• Unnamed Item
• Particle creation by black holes
• Microscopic origin of the Bekenstein-Hawking entropy
• The four laws of black hole mechanics
• Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
• Quantum Geometry and Black Hole Entropy
• The singularities of gravitational collapse and cosmology
• THE CASE FOR DISCRETE ENERGY LEVELS OF A BLACK HOLE
• Black Holes and Entropy
• Quantum gravity and Regge calculus
• Black hole mass spectrum vs spectrum of Hawking radiation

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