dc.contributor.author |
Bhattacharya, Aranya |
|
dc.contributor.author |
Bhattacharyya, Arpan |
|
dc.contributor.author |
Patra, Ayan K. |
|
dc.coverage.spatial |
United Kingdom |
|
dc.date.accessioned |
2023-07-28T15:18:23Z |
|
dc.date.available |
2023-07-28T15:18:23Z |
|
dc.date.issued |
2023-07 |
|
dc.identifier.citation |
Bhattacharya, Aranya; Bhattacharyya, Arpan and Patra, Ayan K., "Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld", Journal of High Energy Physics, DOI: 10.1007/JHEP07(2023)060, vol. 2023, no. 7, Jul. 2023. |
|
dc.identifier.issn |
1126-6708 |
|
dc.identifier.issn |
1029-8479 |
|
dc.identifier.uri |
https://doi.org/10.1007/JHEP07(2023)060 |
|
dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/9050 |
|
dc.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 Phi, 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. |
|
dc.description.statementofresponsibility |
by Aranya Bhattacharya, Arpan Bhattacharyya and Ayan K. Patra |
|
dc.format.extent |
vol. 2023, no. 7 |
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dc.language.iso |
en_US |
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dc.publisher |
Springer |
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dc.subject |
2D gravity |
|
dc.subject |
AdS-CFT correspondence |
|
dc.subject |
Black holes in string theory |
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dc.subject |
Models of quantum gravity |
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dc.subject |
Holographic complexity |
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dc.title |
Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld |
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dc.type |
Article |
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dc.relation.journal |
Journal of High Energy Physics |
|