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Seminar
Speaker
Geoffrey Penington (Stanford University)
Date & Time
Wed, 24 June 2020, 09:00 to 10:30
Venue
ICTS virtual seminar, Please use the link to join the meeting: https://zoom.us/j/96113616930?pwd=UVIxbjY4SzF2aTBLMnpGeGNQNFBrUT09. (Meeting ID: 961 1361 6930 Password: 1y0fG8)
Resources
Abstract

Hawking famously argued, based on semiclassical calculations, that the radiation from evaporating black holes is always perfectly thermal and contains no information about the matter that fell in. Such a result is inconsistent with the unitarity of quantum mechanics. In this talk, I will argue that a more careful replica trick calculation shows that the gravitational path integral becomes dominated at late times by saddles containing spacetime wormholes. These wormholes cause the entropy to decrease after the Page time, consistent with unitarity, and allow information to escape from the interior of the black hole. In very simple toy models, we can evaluate the path integral exactly, and see the information emerge. In more realistic black holes, the full wormhole solutions cannot be found explicitly. However, their existence, and their most important consequences, can be derived by studying the location and properties of a non-trivial ‘quantum extremal surface’ in the original Hawking solution.

Recordings of past talks can be found here: www.youtube.com/channel/UCw9LdPQ5t7Q7muD0qzn70TA