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

Aranya Bhattacharya; Arpan Bhattacharyya; Ayan K. Patra

doi:10.1007/JHEP07(2023)060

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

Aranya Bhattacharya, Arpan Bhattacharyya, Ayan K. Patra^*

^*Corresponding author for this work

School of Mathematics

Research output: Contribution to journal › Article (Academic Journal) › peer-review

13 Citations (Scopus)

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 φ0, 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.

Original language	English
Article number	60
Number of pages	24
Journal	JHEP
Volume	2023
Issue number	7
DOIs	https://doi.org/10.1007/JHEP07(2023)060
Publication status	Published - 7 Jul 2023

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Publisher Copyright:
© The Authors. Article funded by SCOAP3.

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hep-th

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Cite this

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title = "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 {\textquoteleft}complexity=volume{\textquoteright} 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 φ0, 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.",

keywords = "hep-th",

author = "Aranya Bhattacharya and Arpan Bhattacharyya and Patra, \{Ayan K.\}",

note = "Publisher Copyright: {\textcopyright} The Authors. Article funded by SCOAP3.",

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TY - JOUR

T1 - Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld

AU - Bhattacharya, Aranya

AU - Bhattacharyya, Arpan

AU - Patra, Ayan K.

PY - 2023/7/7

Y1 - 2023/7/7

N2 - 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 φ0, 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.

AB - 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 φ0, 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.

KW - hep-th

U2 - 10.1007/JHEP07(2023)060

DO - 10.1007/JHEP07(2023)060

M3 - Article (Academic Journal)

SN - 1029-8479

VL - 2023

JO - JHEP

JF - JHEP

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M1 - 60

ER -