Holography at Finite N: Breakdown of Bulk Reconstruction for Subregions

Fuente: arXiv
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Main Author: Terashima, Seiji
Format: Preprint
Published: 2025
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author Terashima, Seiji
author_facet Terashima, Seiji
contents Within AdS/CFT, focusing on the AdS-Rindler wedge, we show that when $N$ is large but finite, correlation functions of reconstructed bulk operators grow exponentially with bulk momentum, overwhelming the usual $1/N$ suppression. The growth starts when the smeared operator's ultraviolet scale goes beyond a critical value $Λ_{crit} = \frac{2}π\ln N$, which is far below the Planck scale. Above this logarithmic threshold, the large $N$ expansion ceases to be reliable, and the would-be bulk operators cannot be consistently defined as observables in the full quantum gravity theory. Since the AdS-Rindler wedge describes the near-horizon region of black holes, this result implies a sharp $\ln N$ cutoff for reconstructing bulk operators across horizons. This has a direct impact on whether and how information from the black hole interior is encoded-a central question in the black hole information paradox.
format Preprint
id arxiv_https___arxiv_org_abs_2508_11592
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Holography at Finite N: Breakdown of Bulk Reconstruction for Subregions
Terashima, Seiji
High Energy Physics - Theory
Within AdS/CFT, focusing on the AdS-Rindler wedge, we show that when $N$ is large but finite, correlation functions of reconstructed bulk operators grow exponentially with bulk momentum, overwhelming the usual $1/N$ suppression. The growth starts when the smeared operator's ultraviolet scale goes beyond a critical value $Λ_{crit} = \frac{2}π\ln N$, which is far below the Planck scale. Above this logarithmic threshold, the large $N$ expansion ceases to be reliable, and the would-be bulk operators cannot be consistently defined as observables in the full quantum gravity theory. Since the AdS-Rindler wedge describes the near-horizon region of black holes, this result implies a sharp $\ln N$ cutoff for reconstructing bulk operators across horizons. This has a direct impact on whether and how information from the black hole interior is encoded-a central question in the black hole information paradox.
title Holography at Finite N: Breakdown of Bulk Reconstruction for Subregions
topic High Energy Physics - Theory
url https://arxiv.org/abs/2508.11592