| dc.contributor.author |
Bhattacharya, Aranya |
|
| dc.contributor.author |
Bhattacharyya, Arpan |
|
| dc.contributor.author |
Patra, Ayan K. |
|
| dc.coverage.spatial |
United States of America |
|
| dc.date.accessioned |
2023-05-17T08:16:05Z |
|
| dc.date.available |
2023-05-17T08:16:05Z |
|
| dc.date.issued |
2023-04 |
|
| dc.identifier.citation |
Bhattacharya, Aranya; Bhattacharyya, Arpan and Patra, Ayan K., "Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld", arXiv, Cornell University Library, DOI: arXiv:2304.09909v1, Apr. 2023. |
|
| dc.identifier.uri |
https://arxiv.org/abs/2304.09909v1 |
|
| dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/8811 |
|
| 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 theholographic 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 ?0, similar to the answer found in [2]. However, in addition, we find subleading corrections to the complexity solely rising from the fluctuations of these Karch-Randall branes. |
|
| dc.description.statementofresponsibility |
by Aranya Bhattacharya, Arpan Bhattacharyya and Ayan K. Patra |
|
| dc.language.iso |
en_US |
|
| dc.publisher |
Cornell University Library |
|
| dc.subject |
Holographic complexity |
|
| dc.subject |
Jackiw-Teitelboim gravity |
|
| dc.subject |
Karch-Randall braneworld |
|
| dc.subject |
Einstein-Hilbert gravity |
|
| dc.subject |
Boundary field theory |
|
| dc.title |
Holographic complexity of Jackiw-Teitelboim gravity from Karch-Randall braneworld |
|
| dc.type |
Article |
|
| dc.relation.journal |
arXiv |
|