Abstract
The prevalent view that evaporating black holes should simply be smaller black holes has been challenged by the firewall paradox. In particular, this paradox suggests that something different occurs once a black hole has evaporated to one-half its original surface area. Here we derive variations of the firewall paradox by tracking the thermodynamic entropy within a black hole across its entire lifetime and extend it even to AdS spacetimes. Our approach sweeps away many unnecessary assumptions, allowing us to demonstrate a paradox exists even after its initial onset (when conventional assumptions render earlier analyses invalid). The most natural resolution may be to accept firewalls as a real phenomenon. Further, the vast entropy accumulated implies a deep firewall that goes “all the way down” in contrast to earlier work describing only a structure at the horizon.
Original language | English |
---|---|
Article number | 20170324 |
Number of pages | 13 |
Journal | PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES |
Volume | 376 |
Issue number | 2123 |
Early online date | 28 May 2018 |
DOIs | |
Publication status | Published - 13 Jul 2018 |
Bibliographical note
© The Authors, 2018.Keywords
- Black holes
- Energetic curtains
- Firewall