Entanglement entropy and its linear response following a global quench in holographic Gauss-Bonnet gravity

Growth of entanglement entropy in time-dependent states formed due to a global quench in holographic conformal field theories which admit an Einstein-Gauss-Bonnet dual gravity description is studied. The global quench in the bulk is modelled by an AdS-Vaidya solution with an electric charge. It is observed that the Gauss-Bonnet correction parameter leads to faster thermalization, and lower saturation entropy. The rate of growth also depends crucially on the correction, and may exceed 1 in general spacetime dimensions. Nevertheless, the growth still follows the universal pattern expected for relativistic CFTs. Additionally, a time-dependent analogue of relative entropy introduced in [1] is generalized to include correction from the Gauss-Bonnet parameter. We demonstrate our findings through concrete examples, including instantaneous, linear, and periodically driven quenches. We also briefly mention the evolution of mutual information.

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Publication Details

Journal
Nuclear Physics B
Published
2025-08-25
DOI
https://doi.org/10.1016/j.nuclphysb.2025.117084
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Entanglement entropy and its linear response following a global quench in holographic Gauss-Bonnet gravity

Sharareh Mehrabi Pari, Sabyasachi Maulik
Nuclear Physics B
Black Holes and Theoretical Physics
article

Entanglement entropy and its linear response following a global quench in holographic Gauss-Bonnet gravity

Sharareh Mehrabi Pari, Sabyasachi Maulik
article en

Abstract

Growth of entanglement entropy in time-dependent states formed due to a global quench in holographic conformal field theories which admit an Einstein-Gauss-Bonnet dual gravity description is studied. The global quench in the bulk is modelled by an AdS-Vaidya solution with an electric charge. It is observed that the Gauss-Bonnet correction parameter leads to faster thermalization, and lower saturation entropy. The rate of growth also depends crucially on the correction, and may exceed 1 in general spacetime dimensions. Nevertheless, the growth still follows the universal pattern expected for relativistic CFTs. Additionally, a time-dependent analogue of relative entropy introduced in [1] is generalized to include correction from the Gauss-Bonnet parameter. We demonstrate our findings through concrete examples, including instantaneous, linear, and periodically driven quenches. We also briefly mention the evolution of mutual information.

Nuclear Physics BVol. 1018
Department of Atomic Energy, Government of India, Nuclear Physics
Openalex Percentile: Top 91%
Black Holes and Theoretical Physics
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Entanglement entropy and its linear response following a global quench in holographic Gauss-Bonnet gravity — Sharareh Mehrabi Pari, Sabyasachi Maulik · Nuclear Physics B (2025) | TGRS Research Map | TGRS