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 anti-de Sitter space–times. 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 with earlier work describing only a structure at the horizon.
This article is part of a discussion meeting issue ‘Foundations of quantum mechanics and their impact on contemporary society’.
Subject
General Physics and Astronomy,General Engineering,General Mathematics
Cited by
3 articles.
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