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...
| Κύριοι συγγραφείς: | , |
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| Μορφή: | Journal (paper) |
| Γλώσσα: | English |
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2018
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| Διαθέσιμο Online: | https://doi.org/10.1007/JHEP01(2016)144 http://hdl.handle.net/10889/11479 |
