Holographic banners

A bstract This paper is concerned with eternal AdS black holes. The quantum cosmological future and past interior states of the black hole may be placed on an equal footing to the left and right AdS boundary data by considering the on-shell bulk action as a function of the left/right/future/past data: S [ ϕ (0) L , ϕ (0) R , ϕ (0) F , ϕ (0) P ]. We call this object a holographic banner, and it obeys the Hamilton-Jacobi equation with respect to all four of its arguments. We compute the holographic banner for a scalar field in an AdS black hole background explicitly and use it to construct the semiclassical state in the future interior obtained from a thermofield double state in the past evolved by arbitrary time- and space-dependent boundary sources. When the spacetime itself is dynamical we explain how the holographic banner gives, in principle, a map from boundary data to near-singularity semiclassical quantum cosmology following chaotic BKL dynamics. We obtain the timescale for ergodic mixing under the future interior BKL dynamics due to a quantum variance in the past state or a classical ensemble of boundary theories.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-08-14
DOI
https://doi.org/10.1007/jhep08(2026)113
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Holographic banners

Matthew J. Blacker, Sean A. Hartnoll
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

Holographic banners

Matthew J. Blacker, Sean A. Hartnoll
article en

Abstract

A bstract This paper is concerned with eternal AdS black holes. The quantum cosmological future and past interior states of the black hole may be placed on an equal footing to the left and right AdS boundary data by considering the on-shell bulk action as a function of the left/right/future/past data: S [ ϕ (0) L , ϕ (0) R , ϕ (0) F , ϕ (0) P ]. We call this object a holographic banner, and it obeys the Hamilton-Jacobi equation with respect to all four of its arguments. We compute the holographic banner for a scalar field in an AdS black hole background explicitly and use it to construct the semiclassical state in the future interior obtained from a thermofield double state in the past evolved by arbitrary time- and space-dependent boundary sources. When the spacetime itself is dynamical we explain how the holographic banner gives, in principle, a map from boundary data to near-singularity semiclassical quantum cosmology following chaotic BKL dynamics. We obtain the timescale for ergodic mixing under the future interior BKL dynamics due to a quantum variance in the past state or a classical ensemble of boundary theories.

Journal of High Energy PhysicsVol. 2026(8)
University of Cambridge (GB)
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Openalex Percentile: Top 66%
Black Holes and Theoretical Physics
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