Islands and complexity of eternal black hole and radiation subsystems for a doubly holographic model

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dc.contributor.author Bhattacharya, Aranya
dc.contributor.author Bhattacharyya, Arpan
dc.contributor.author Nandy, Pratik
dc.contributor.author Patra, Ayan K
dc.date.accessioned 2021-05-14T05:18:45Z
dc.date.available 2021-05-14T05:18:45Z
dc.date.issued 2021-03
dc.identifier.citation Bhattacharya, Aranya; Bhattacharyya, Arpan; Nandy, Pratik and Patra, Ayan K., "Islands and complexity of eternal black hole and radiation subsystems for a doubly holographic model", arXiv, Cornell University Library, DOI: arXiv:/2103.15852, Mar. 2021. en_US
dc.identifier.uri http://arxiv.org/abs/2103.15852
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/6466
dc.description.abstract We study the entanglement islands and subsystem volume complexity corresponding to the left/ right entanglement of a conformal defect in d-dimensions in Randall-Sundrum (RS) braneworld model with subcritical tension brane. The left and right modes of the defect mimic the eternal black hole and radiation system respectively. Hence the entanglement entropy between the two follows an eternal black hole Page curve which is unitarity compatible. We compute the volumes corresponding to the left and right branes with preferred Ryu-Takanayagi (RT) surfaces at different times, which provide a probe of the subregion complexity of the black hole and the radiation states respectively. An interesting jump in volume is found at Page time, where the entanglement curve is saturated due to the inclusion of the island surfaces. We explain various possibilities of this phase transition in complexity at Page time and argue how these results match with a covariant proposal qualitatively.
dc.description.statementofresponsibility by Aranya Bhattacharya, Arpan Bhattacharyya, Pratik Nandy and Ayan K. Patra
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.title Islands and complexity of eternal black hole and radiation subsystems for a doubly holographic model en_US
dc.type Pre-Print en_US
dc.relation.journal arXiv


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