Finite cutoff JT gravity: Baby universes, Matrix dual, and (Krylov) Complexity

Fuente: arXiv
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Autores principales: Bhattacharyya, Arpan, Ghosh, Saptaswa, Pal, Sounak, Vinod, Anandu
Formato: Preprint
Publicado: 2025
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author Bhattacharyya, Arpan
Ghosh, Saptaswa
Pal, Sounak
Vinod, Anandu
author_facet Bhattacharyya, Arpan
Ghosh, Saptaswa
Pal, Sounak
Vinod, Anandu
contents In this paper, as an application of the `Complexity = Volume' proposal, we calculate the growth of the interior of a black hole at late times for finite cutoff JT gravity. Due to this integrable, irrelevant deformation, the spectral properties are modified non-trivially. The Einstein-Rosen Bridge (ERB) length saturates faster than pure JT gravity. We comment on the possible connection between Krylov Complexity and ERB length for the deformed theory. Apart from this, we compute the emission probability of baby universes in the deformed theory and find that it changes due to the deformation parameter only if we turn on Lorentzian evolution. We also find that the saturation time of the deformed theory relative to the undeformed one depends on the inverse temperature. We also highlight the subtleties involved in the dual matrix model and comment on the possible one-cut universality. Finally, we comment on the possible correction to the volume of the moduli space arising from the non-perturbative correction of the spectral curve induced by the finite boundary cutoff.
format Preprint
id arxiv_https___arxiv_org_abs_2502_13208
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Finite cutoff JT gravity: Baby universes, Matrix dual, and (Krylov) Complexity
Bhattacharyya, Arpan
Ghosh, Saptaswa
Pal, Sounak
Vinod, Anandu
High Energy Physics - Theory
General Relativity and Quantum Cosmology
Mathematical Physics
Quantum Physics
In this paper, as an application of the `Complexity = Volume' proposal, we calculate the growth of the interior of a black hole at late times for finite cutoff JT gravity. Due to this integrable, irrelevant deformation, the spectral properties are modified non-trivially. The Einstein-Rosen Bridge (ERB) length saturates faster than pure JT gravity. We comment on the possible connection between Krylov Complexity and ERB length for the deformed theory. Apart from this, we compute the emission probability of baby universes in the deformed theory and find that it changes due to the deformation parameter only if we turn on Lorentzian evolution. We also find that the saturation time of the deformed theory relative to the undeformed one depends on the inverse temperature. We also highlight the subtleties involved in the dual matrix model and comment on the possible one-cut universality. Finally, we comment on the possible correction to the volume of the moduli space arising from the non-perturbative correction of the spectral curve induced by the finite boundary cutoff.
title Finite cutoff JT gravity: Baby universes, Matrix dual, and (Krylov) Complexity
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
Mathematical Physics
Quantum Physics
url https://arxiv.org/abs/2502.13208