Distinguishing Random and Black Hole Microstates
Jonah Kudler-Flam, Vladimir Narovlansky, Shinsei Ryu

TL;DR
This paper advances the understanding of black hole microstates and random states by computing generalized entropies and distances, revealing new structures and implications for the black hole information paradox.
Contribution
It introduces generalized entropy measures for black hole microstates and random tensor networks, connecting these to holography and quantum hypothesis testing.
Findings
Generalized entropies distinguish black hole microstates more effectively.
New phenomena in random tensor networks relate to holographic states.
Chaotic systems obey subsystem ETH for subsystems less than half the total size.
Abstract
This is an expanded version of the short report [Phys. Rev. Lett. 126, 171603 (2021)], where the relative entropy was used to distinguish random states drawn from the Wishart ensemble as well as black hole microstates. In this work, we expand these ideas by computing many generalizations including the Petz R\'enyi relative entropy, sandwiched R\'enyi relative entropy, fidelities, and trace distances. These generalized quantities are able to teach us about new structures in the space of random states and black hole microstates where the von Neumann and relative entropies were insufficient. We further generalize to generic random tensor networks where new phenomena arise due to the locality in the networks. These phenomena sharpen the relationship between holographic states and random tensor networks. We discuss the implications of our results on the black hole information problem using…
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