Holographic Black Hole Formation and Scrambling in Time-Ordered Correlators

We describe a holographic mechanism for black hole formation via the collision of two shock waves in three-dimensional anti–de Sitter spacetime. In the dual conformal field theory, a two-shock-wave state corresponds to the insertion of two boosted “precursor” operators in complementary Rindler patches. Their operator product expansion is initially described by a universal mean-field spectrum of exchanged states, which is dominated by operator dimensions that grow exponentially in the boost parameter. We propose their mean value as diagnosing the mass of the collision product in the bulk. It crosses the conformal field theory heavy state threshold after two scrambling times, in accordance with expectations about black hole formation in general relativity. Our analysis also allows us to identify the scrambling characteristics usually associated with out-of-time-order correlation functions, using only the internal composition of thermal in-time-order correlators.

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Publication Details

Journal
Physical Review Letters
Published
2026-02-12
DOI
https://doi.org/10.1103/ywfb-82lh
Primary Topic
Theoretical and Computational Physics
Type
article
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article

Holographic Black Hole Formation and Scrambling in Time-Ordered Correlators

Anonymous
Physical Review Letters
Theoretical and Computational Physics
article

Holographic Black Hole Formation and Scrambling in Time-Ordered Correlators

Anonymous
article en

Abstract

We describe a holographic mechanism for black hole formation via the collision of two shock waves in three-dimensional anti–de Sitter spacetime. In the dual conformal field theory, a two-shock-wave state corresponds to the insertion of two boosted “precursor” operators in complementary Rindler patches. Their operator product expansion is initially described by a universal mean-field spectrum of exchanged states, which is dominated by operator dimensions that grow exponentially in the boost parameter. We propose their mean value as diagnosing the mass of the collision product in the bulk. It crosses the conformal field theory heavy state threshold after two scrambling times, in accordance with expectations about black hole formation in general relativity. Our analysis also allows us to identify the scrambling characteristics usually associated with out-of-time-order correlation functions, using only the internal composition of thermal in-time-order correlators.

Physical Review LettersVol. 136(12)
University of Southampton (GB), Massachusetts Institute of Technology (US)
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Openalex Percentile: Top 56%
Theoretical and Computational Physics
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Holographic Black Hole Formation and Scrambling in Time-Ordered Correlators — Anonymous · Physical Review Letters (2026) | TGRS Research Map | TGRS