The thermodynamics of a black hole in equilibrium implies the breakdown of Einstein equations on a macroscopic near-horizon shell

DOI10.1007/JHEP01(2016)144zbMath1388.83367arXiv1410.0788OpenAlexW2396590333MaRDI QIDQ1638174

Charis Anastopoulos, Ntina Savvidou

Publication date: 12 June 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1410.0788

zbMATH Keywords

black holesclassical theories of gravity

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

Related Items (3)

Thermodynamics of spherically symmetric thin-shell spacetimes ⋮ 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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• The thermodynamics of self-gravitating systems in equilibrium is holographic
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