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Holographic Entanglement Entropy of the BTZ Black Hole

2009/07/22 by Mariano Cadoni, M. Cadoni, Maurizio Melis +1 · 1 citation
Physics and Astronomy · #BTZ black hole #Black Holes and Theoretical Physics #Black brane #Black hole thermodynamics #Classical mechanics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Extremal black hole #Holography #Noncommutative and Quantum Gravity Theories #Physics #Quantum #Quantum entanglement #Quantum mechanics #Theoretical physics #hep-th

paper · pdf · doi:10.1007/s10701-010-9430-6

published as Found.Phys.40:638-657,2010 · We added the comparison of some of our results with previous results for the quantum entropy of a scalar in the Euclidean BTZ background. Two more references have been also added

arxiv created 2009/07/22 · openalex publication_date 2010/02/11 · arxiv updated 2014/11/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We investigate quantum entanglement of gravitational configurations in 3D AdS gravity using the AdS/CFT correspondence. We derive explicit formulas for the holographic entanglement entropy (EE) of the BTZ black hole, conical singularities and regularized AdS3. The leading term in the large temperature expansion of the holographic EE of the BTZ black hole reproduces exactly its Bekenstein-Hawking entropy SBH, whereas the subleading term behaves as ln SBH. We also show that the leading term of the holographic EE for the BTZ black hole can be obtained from the large temperature expansion of the partition function of a broad class of 2D CFTs on the torus. This result indicates that black hole EE is not a fundamental feature of the underlying theory of quantum gravity but emerges when the semiclassical notion of spacetime geometry is used to describe the black hole.

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