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

We study a black hole of mass M, enclosed within a spherical box, in equilibrium with its Hawking radiation. We show that the spacetime geometry inside the box is described by the Oppenheimer-Volkoff equations for radiation, except for a {\em thin shell} around the horizon. We use the maximum entrop...

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Bibliographic Details
Main Authors: Anastopoulos, Charis, Savvidou, Ntina
Other Authors: Αναστασόπουλος, Χάρης
Format: Journal (paper)
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2016)144
http://hdl.handle.net/10889/11479