The thermodynamics of self-gravitating systems in equilibrium is holographic
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Publication:5413600
DOI10.1088/0264-9381/31/5/055003zbMath1292.83013arXiv1302.4407OpenAlexW3103701017MaRDI QIDQ5413600
Ntina Savvidou, Charis Anastopoulos
Publication date: 30 April 2014
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1302.4407
Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classical and relativistic thermodynamics (80A10) Measures of information, entropy (94A17)
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The thermodynamics of a black hole in equilibrium implies the breakdown of Einstein equations on a macroscopic near-horizon shell ⋮ Thermodynamics of spherically symmetric thin-shell spacetimes ⋮ Black holes and hot shells in the Euclidean path integral approach to quantum gravity ⋮ Gravitational potential from maximum entropy principle ⋮ Classification theorem and properties of singular solutions to the Tolman–Oppenheimer–Volkoff equation ⋮ Thermodynamics and phase transitions of black holes in contact with a gravitating heat bath
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