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Chaos in the black hole S-matrix

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it
abstract

Recent work by Shenker, Stanford, and Kitaev has related the black hole horizon geometry to chaotic behavior. We extend this from eternal black holes to black holes that form and then evaporate. This leads to an identity for the change in the black hole S-matrix (over times shorter than the scrambling time) due an addition infalling particle, elaborating an idea of 't Hooft.

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2026 3 2024 1

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Many-Body Quantum Chaos At All Time Scales

hep-th · 2026-05-26 · unverdicted · novelty 7.0

Analytical all-time expressions for Green's and OTOC functions in 4-body SYK model show early exponential growth then decay, followed by late-time dip-ramp-plateau patterns deviating from ergodic predictions due to local energy correlations for N mod 8 = 2,6.

Long-time Freeness in the Kicked Top

cond-mat.stat-mech · 2024-11-18 · unverdicted · novelty 6.0

In the fully chaotic regime of the kicked top, long-time freeness is reached exponentially fast, accompanied by a hierarchy of time scales indicating a multifractal approach.

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