Learning the Alpha-bits of black holes

Abstract When the bulk geometry in AdS/CFT contains a black hole, boundary subregions may be sufficient to reconstruct certain bulk operators if and only if the black hole microstate is known, an example of state dependence. Reconstructions exist for any microstate, but no reconstruction works for a...

Full description

Bibliographic Details
Main Authors: Patrick Hayden, Geoffrey Penington
Format: Article
Language:English
Published: SpringerOpen 2019-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2019)007
_version_ 1818602599008436224
author Patrick Hayden
Geoffrey Penington
author_facet Patrick Hayden
Geoffrey Penington
author_sort Patrick Hayden
collection DOAJ
description Abstract When the bulk geometry in AdS/CFT contains a black hole, boundary subregions may be sufficient to reconstruct certain bulk operators if and only if the black hole microstate is known, an example of state dependence. Reconstructions exist for any microstate, but no reconstruction works for all microstates. We refine this dichotomy, demonstrating that the same boundary operator can often be used for large subspaces of black hole microstates, corresponding to a constant fraction α of the black hole entropy. In the Schrödinger picture, the boundary subregion encodes the α-bits (a concept from quantum information) of a bulk region containing the black hole and bounded by extremal surfaces. These results have important consequences for the structure of AdS/CFT and for quantum information. Firstly, they imply that the bulk reconstruction is necessarily only approximate and allow us to place non-perturbative lower bounds on the error when doing so. Second, they provide a simple and tractable limit in which the entanglement wedge is state dependent, but in a highly controlled way. Although the state dependence of operators comes from ordinary quantum error correction, there are clear connections to the Papadodimas-Raju proposal for understanding operators behind black hole horizons. In tensor network toy models of AdS/CFT, we see how state dependence arises from the bulk operator being ‘pushed’ through the black hole itself. Finally, we show that black holes provide the first ‘explicit’ examples of capacity-achieving α-bit codes. Unintuitively, Hawking radiation always reveals the α-bits of a black hole as soon as possible. In an appendix, we apply a result from the quantum information literature to prove that entanglement wedge reconstruction can be made exact to all orders in 1/N.
first_indexed 2024-12-16T13:09:50Z
format Article
id doaj.art-0a729269df2f41a49ceb090293d7a423
institution Directory Open Access Journal
issn 1029-8479
language English
last_indexed 2024-12-16T13:09:50Z
publishDate 2019-12-01
publisher SpringerOpen
record_format Article
series Journal of High Energy Physics
spelling doaj.art-0a729269df2f41a49ceb090293d7a4232022-12-21T22:30:38ZengSpringerOpenJournal of High Energy Physics1029-84792019-12-0120191215510.1007/JHEP12(2019)007Learning the Alpha-bits of black holesPatrick Hayden0Geoffrey Penington1Stanford Institute for Theoretical Physics, Stanford UniversityStanford Institute for Theoretical Physics, Stanford UniversityAbstract When the bulk geometry in AdS/CFT contains a black hole, boundary subregions may be sufficient to reconstruct certain bulk operators if and only if the black hole microstate is known, an example of state dependence. Reconstructions exist for any microstate, but no reconstruction works for all microstates. We refine this dichotomy, demonstrating that the same boundary operator can often be used for large subspaces of black hole microstates, corresponding to a constant fraction α of the black hole entropy. In the Schrödinger picture, the boundary subregion encodes the α-bits (a concept from quantum information) of a bulk region containing the black hole and bounded by extremal surfaces. These results have important consequences for the structure of AdS/CFT and for quantum information. Firstly, they imply that the bulk reconstruction is necessarily only approximate and allow us to place non-perturbative lower bounds on the error when doing so. Second, they provide a simple and tractable limit in which the entanglement wedge is state dependent, but in a highly controlled way. Although the state dependence of operators comes from ordinary quantum error correction, there are clear connections to the Papadodimas-Raju proposal for understanding operators behind black hole horizons. In tensor network toy models of AdS/CFT, we see how state dependence arises from the bulk operator being ‘pushed’ through the black hole itself. Finally, we show that black holes provide the first ‘explicit’ examples of capacity-achieving α-bit codes. Unintuitively, Hawking radiation always reveals the α-bits of a black hole as soon as possible. In an appendix, we apply a result from the quantum information literature to prove that entanglement wedge reconstruction can be made exact to all orders in 1/N.https://doi.org/10.1007/JHEP12(2019)007AdS-CFT CorrespondenceGauge-gravity correspondence
spellingShingle Patrick Hayden
Geoffrey Penington
Learning the Alpha-bits of black holes
Journal of High Energy Physics
AdS-CFT Correspondence
Gauge-gravity correspondence
title Learning the Alpha-bits of black holes
title_full Learning the Alpha-bits of black holes
title_fullStr Learning the Alpha-bits of black holes
title_full_unstemmed Learning the Alpha-bits of black holes
title_short Learning the Alpha-bits of black holes
title_sort learning the alpha bits of black holes
topic AdS-CFT Correspondence
Gauge-gravity correspondence
url https://doi.org/10.1007/JHEP12(2019)007
work_keys_str_mv AT patrickhayden learningthealphabitsofblackholes
AT geoffreypenington learningthealphabitsofblackholes