Trapping, chaos and averaging in bubbling AdS spaces

A bstract We discuss chaos and ensemble averaging in 1/2 BPS bubbling AdS spaces of Lin, Lunin and Maldacena (LLM) by studying trapped and escaping null geodesics and estimating their decay rates. We find typical chaotic scattering behavior and confirm the Pesin relation between escape rates, Lyapunov exponents and Kolmogorov-Sinai entropy. On the other hand, for geodesics in coarse-grained (grayscale) LLM geometries (which exhibit a naked singularity) chaos is strongly suppressed, which is consistent with orbits and escape rates averaged over microscopic backgrounds. Also the singularities in these grayscale geometries produce an attractive potential and have some similarities to black hole throats trapping geodesics for a long time. Overall, averaging over the ensembles of LLM geometries brings us closer toward the typical behavior of geodesics in black hole backgrounds, but some important differences remain, in particular the existence of a threshold timescale when the averaging fails.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-02-16
DOI
https://doi.org/10.1007/jhep02(2026)157
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Trapping, chaos and averaging in bubbling AdS spaces

Vladan Ðukić, David Berenstein, Mihailo Čubrović
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

Trapping, chaos and averaging in bubbling AdS spaces

Vladan Ðukić, David Berenstein, Mihailo Čubrović
article en

Abstract

A bstract We discuss chaos and ensemble averaging in 1/2 BPS bubbling AdS spaces of Lin, Lunin and Maldacena (LLM) by studying trapped and escaping null geodesics and estimating their decay rates. We find typical chaotic scattering behavior and confirm the Pesin relation between escape rates, Lyapunov exponents and Kolmogorov-Sinai entropy. On the other hand, for geodesics in coarse-grained (grayscale) LLM geometries (which exhibit a naked singularity) chaos is strongly suppressed, which is consistent with orbits and escape rates averaged over microscopic backgrounds. Also the singularities in these grayscale geometries produce an attractive potential and have some similarities to black hole throats trapping geodesics for a long time. Overall, averaging over the ensembles of LLM geometries brings us closer toward the typical behavior of geodesics in black hole backgrounds, but some important differences remain, in particular the existence of a threshold timescale when the averaging fails.

Journal of High Energy PhysicsVol. 2026(2)
University of California System (US), University of Belgrade (RS), Delta Institute for Theoretical Physics (NL), University of Amsterdam (NL)
U.S. Department of Energy, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Ministarstvo Prosvete, Nauke i Tehnološkog Razvoja, Russian Science Foundation, Science Fund of the Republic of Serbia
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Openalex Percentile: Top 44%
Black Holes and Theoretical Physics
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