Entanglement dynamics in 2d HCFTs on the curved background: the case of q-Möbius Hamiltonian

A bstract We will explore the dynamical property of non-equilibrium phenomena induced by two-dimensional holographic conformal field theory (2d holographic CFT) Hamiltonian on the curved spacetime by studying the time dependence of the entanglement entropy and mutual information. Here, holographic CFT is the CFT having the gravity dual. We will start from the boundary and thermofield double states, evolve the systems in Euclidean time with the Hamiltonian on the curved background, and then evolve them in real-time with the same Hamiltonian. We found that the early- and late-time entanglement structure depends on the curved background, while the entanglement growth does not, and is linear. Furthermore, in the gravity dual for the thermofield double state, this entanglement growth is due to the linear growth of the wormhole, while in the one for the boundary state, it is due to the in-falling of the end of the world brane to the black hole. We discussed the low temperature system can be regarded as the dynamical system induced by the multi-joining quenches. We also discussed the effective description of the high temperature system, called line tension picture.

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Publication Details

Journal
Journal of High Energy Physics
Published
2024-12-27
DOI
https://doi.org/10.1007/jhep12(2024)208
Citations
9
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
5.94

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article

Entanglement dynamics in 2d HCFTs on the curved background: the case of q-Möbius Hamiltonian

Masahiro Nozaki, Akihiro Miyata, Chen Bai
9 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
5.94
article

Entanglement dynamics in 2d HCFTs on the curved background: the case of q-Möbius Hamiltonian

Masahiro Nozaki, Akihiro Miyata, Chen Bai
article en
9 citations

Abstract

A bstract We will explore the dynamical property of non-equilibrium phenomena induced by two-dimensional holographic conformal field theory (2d holographic CFT) Hamiltonian on the curved spacetime by studying the time dependence of the entanglement entropy and mutual information. Here, holographic CFT is the CFT having the gravity dual. We will start from the boundary and thermofield double states, evolve the systems in Euclidean time with the Hamiltonian on the curved background, and then evolve them in real-time with the same Hamiltonian. We found that the early- and late-time entanglement structure depends on the curved background, while the entanglement growth does not, and is linear. Furthermore, in the gravity dual for the thermofield double state, this entanglement growth is due to the linear growth of the wormhole, while in the one for the boundary state, it is due to the in-falling of the end of the world brane to the black hole. We discussed the low temperature system can be regarded as the dynamical system induced by the multi-joining quenches. We also discussed the effective description of the high temperature system, called line tension picture.

Journal of High Energy PhysicsVol. 2024(12)
Kavli Institute for Theoretical Sciences (CN), RIKEN (JP), University of Chinese Academy of Sciences (CN)
Chinese Academy of Sciences, University of Chinese Academy of Sciences
Openalex Percentile: Top 3%
Black Holes and Theoretical Physics
5.94
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