Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld

Abstract Recently, it has been argued in [1] that Jackiw-Teitelboim (JT) gravity can be naturally realized in the Karch-Randall braneworld in (2 + 1) dimensions. Using the ‘complexity=volume’ proposal, we studied this model and computed the holographic complexity of the JT gravity from the bulk pers...

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Main Authors: Aranya Bhattacharya, Arpan Bhattacharyya, Ayan K. Patra
Format: Article
Language:English
Published: SpringerOpen 2023-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP07(2023)060
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author Aranya Bhattacharya
Arpan Bhattacharyya
Ayan K. Patra
author_facet Aranya Bhattacharya
Arpan Bhattacharyya
Ayan K. Patra
author_sort Aranya Bhattacharya
collection DOAJ
description Abstract Recently, it has been argued in [1] that Jackiw-Teitelboim (JT) gravity can be naturally realized in the Karch-Randall braneworld in (2 + 1) dimensions. Using the ‘complexity=volume’ proposal, we studied this model and computed the holographic complexity of the JT gravity from the bulk perspective. We find that the complexity grows linearly with boundary time at late times, and the leading order contribution is proportional to the φ 0, similar to the answer found in [2]. However, in addition, we find subleading corrections to the complexity solely arising from the fluctuations of these Karch-Randall branes.
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spelling doaj.art-a268869cf72c4d0c850bbaee4c0f469f2023-10-29T12:09:24ZengSpringerOpenJournal of High Energy Physics1029-84792023-07-012023712410.1007/JHEP07(2023)060Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworldAranya Bhattacharya0Arpan Bhattacharyya1Ayan K. Patra2Centre for High Energy Physics, Indian Institute of ScienceIndian Institute of TechnologyInstituto de Física Teorica UAM/CSICAbstract Recently, it has been argued in [1] that Jackiw-Teitelboim (JT) gravity can be naturally realized in the Karch-Randall braneworld in (2 + 1) dimensions. Using the ‘complexity=volume’ proposal, we studied this model and computed the holographic complexity of the JT gravity from the bulk perspective. We find that the complexity grows linearly with boundary time at late times, and the leading order contribution is proportional to the φ 0, similar to the answer found in [2]. However, in addition, we find subleading corrections to the complexity solely arising from the fluctuations of these Karch-Randall branes.https://doi.org/10.1007/JHEP07(2023)0602D GravityAdS-CFT CorrespondenceBlack Holes in String TheoryModels of Quantum Gravity
spellingShingle Aranya Bhattacharya
Arpan Bhattacharyya
Ayan K. Patra
Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
Journal of High Energy Physics
2D Gravity
AdS-CFT Correspondence
Black Holes in String Theory
Models of Quantum Gravity
title Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
title_full Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
title_fullStr Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
title_full_unstemmed Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
title_short Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld
title_sort holographic complexity of jackiw teitelboim gravity from karch randall braneworld
topic 2D Gravity
AdS-CFT Correspondence
Black Holes in String Theory
Models of Quantum Gravity
url https://doi.org/10.1007/JHEP07(2023)060
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