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Holographic thermalization in Gauss-Bonnet gravity with de Sitter boundary

2014/12/31 by Shao-Jun Zhang, Bin Wang, Élcio Abdalla +2 · 2 citations
Physics and Astronomy · #Anti-de Sitter space #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #De Sitter space #De Sitter universe #Entropy (arrow of time) #Gauss–Bonnet theorem #Mathematical physics #Observable #Physics #Quantum #Quantum Electrodynamics and Casimir Effect #Quantum entanglement #Quantum gravity #Quantum mechanics #Thermalisation #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.91.106010

published as Phys. Rev. D 91, 106010 (2015) · 27 pages, 13 figures, minor modifications

arxiv created 2015/05/26 · openalex publication_date 2015/05/26 · arxiv updated 2015/06/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We introduce higher-derivative Gauss-Bonnet correction terms in the gravity sector, and we relate the modified gravity theory in the bulk to the strongly coupled quantum field theory on a de Sitter boundary. We study the process of holographic thermalization by examining three nonlocal observables, the two-point function, the Wilson loop and the holographic entanglement entropy. We study the time evolution of these three observables, and we find that as the strength of the Gauss-Bonnet coupling is increased, the saturation time of the thermalization process to reach thermal equilibrium becomes shorter with the dominant effect given by the holographic entanglement entropy.

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