A covariant holographic entanglement entropy proposal
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The Ryu-Takayanagi formula, including quantum corrections, states that the entanglement entropy of a boundary region B is equal to the generalised entropy of the Ryu-Takayanagi surface.
“The Ryu-Takayanagi formula, including quantum corrections, states that entanglement entropy of the boundary region B is equal to the generalised entropy of the Ryu-Takayanagi surface.”
From Entanglement wedge reconstruction and the information paradox (2020) · cites this paper as [28]
The discussion around eq. (2.2) gives the boundary region’s entanglement entropy as the area of a bulk minimal surface divided by 4G. The paper also discusses quantum corrections to a Bousso entropy bound around eqs. (3.4)–(3.5), but it does not state that the quantum-corrected boundary entropy equals the generalised entropy of an RT surface. The passages in our copy have no page numbers. (LLM, conf=0.88)
Experimental — accuracy not yet measuredIn this way, we obtain the quantum extremal surface prescription of [23], and also [20, 21].
“In this way, we obtain the quantum extremal surface prescription of [23], and also [20, 21].”
From Replica wormholes and the entropy of Hawking radiation (2020) · cites this paper as [21]
Section 3.3, equation (3.15), proposes calculating holographic entanglement entropy from the area of a surface with vanishing null expansions. That supports an extremal-surface prescription, but the passage does not give the quantum extremal-surface prescription claimed here: it extremizes area, not a quantity including bulk entropy. (LLM, conf=0.86)
Experimental — accuracy not yet measuredThe entropy of the black hole is given by the generalized entropy of the quantum extremal surface (QES), a quantum-corrected Ryu-Takayanagi surface.
“The entropy of the black hole is given by the generalized entropy of the quantum extremal surface (QES) [23], which is a quantum-corrected Ryu-Takayanagi (or Hubeny-Rangamani-Takayanagi) surface [20, 21].”
From Replica wormholes and the entropy of Hawking radiation (2020) · cites this paper as [21]
Section 3.3 describes the covariant extremal-surface prescription, supporting the identification of an HRT surface. Section 6.6 relates that surface to the apparent horizon in a limiting case. The cited paper does not state that a quantum extremal surface is obtained by extremizing generalized entropy; the citing sentence assigns the QES entropy claim to a different citation. (LLM, conf=0.88)
Experimental — accuracy not yet measuredThe QRT prescription for entanglement entropy between A and its complement is given by the smallest extremal value of the generalized entropy.
“The QRT prescription for entanglement entropy between A and ¯ A , or in this case the entanglement entropy between the black hole and the Hawking radiation, is then given by the smallest extremal value of (2.1).”
From Page curve for an evaporating black hole (2020) · cites this paper as [8]
Section 3.3, proposal (II) (page not provided), says to choose the minimum-area surface when multiple extremal surfaces satisfy the boundary and homotopy conditions. It gives entropy as area divided by 4G, not as the extremal value of generalized entropy, and does not state this prescription for entanglement between a black hole and its Hawking radiation. (LLM, conf=0.89)
Experimental — accuracy not yet measuredThe Ryu-Takayanagi or covariant Hubeny-Rangamani-Takayanagi prescription computes the entanglement entropy of a spacelike region A in the CFT in the bulk by the area of a codimension-two minimal surface with boundary anchored on the boundary of A.
“This can be explicitly checked with the Ryu-Takayanagi (RT) or the covariant Hubeny-Rangamani-Takayanagi prescription (Ryu and Takayanagi, 2006a,b;Hubeny et al., 2007): The entanglement entropy of a spacelike region A in the CFT is computed in the bulk by the area of a codimension-two minimal surface with boundary anchored on ∂A.”
From Euclidean Wormholes, Baby Universes, and Their Impact on Particle Physics and Cosmology (2018) · cites this paper as Hubeny et al., 2007
The paper’s static prescription describes entanglement entropy using the area of a codimension-two minimal bulk surface anchored on ∂A. Its covariant proposal (section 3.3, equation 3.15; page unavailable) instead uses an extremal surface with vanishing null expansions, choosing the minimum-area surface only among qualifying extremal surfaces. Calling the covariant surface simply a minimal surface omits that distinction. (LLM, conf=0.90)
Experimental — accuracy not yet measured
Since the CFT2 has a holographic dual, the contribution of the χ fields to the entropy can be computed to leading order using the RT/HRT formula.
“Furthermore, since the CFT 2 has a holographic dual, the contribution of the χ fields to the entropy can be computed to leading order using the RT/HRT formula [5,6].”
From The Page curve of Hawking radiation from semiclassical geometry (2020) · cites this paper as [6]
For a two-dimensional black hole coupled to a holographic matter CFT, the quantum extremal surface prescription of [7] reduces to the usual RT/HRT [5,6] prescription in the bulk geometry.
“In this case, the quantum extremal surface prescription of [7] reduces to the usual RT/HRT [5,6] prescription in the bulk geometry.”
From The Page curve of Hawking radiation from semiclassical geometry (2020) · cites this paper as [6]
The RT/HRT formula states that the entanglement entropy of a boundary subregion R is proportional to the area of the classical bulk co-dimension two extremal surface anchored to the boundary of R and homologous to R.
“The RT/HRT formula states that the entanglement entropy of a subregion R of the boundary theory is proportional to the area of the classical, bulk co-dimension two 3extremal surface that is anchored to the boundary of R and is homologous to R (see Fig. 2).”
From Holographic spacetime, black holes and quantum error correcting codes: a review (2022) · cites this paper as [24]
In a gravity theory coupled to matter whose matter has a higher-dimensional holographic dual, finding quantum extremal surfaces is equivalent to finding the RT/HRT surfaces in the higher-dimensional theory.
“In such a theory, finding quantum extremal surfaces becomes equivalent to finding the RT/HRT surfaces in the higher-dimensional theory.”
From The Page curve of Hawking radiation from semiclassical geometry (2020) · cites this paper as [6]
The brane-world discussion (section 3, page unavailable) relates gravity coupled to a QFT to a higher-dimensional bulk calculation of entropy bounds. Section 5.1.2 discusses classical holographic extremal surfaces, but our copy does not address whether finding quantum extremal surfaces is equivalent to finding higher-dimensional RT/HRT surfaces. Searched for quantum extremal surfaces, generalized entropy, holographic matter, and the proposed equivalence. (LLM, conf=0.76)
Experimental — accuracy not yet measured
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“However, for general dynamic spacetimes [27], and taking into account quantum corrections [28, 29], it is the quantum extremal surface, homologous to B, with the smallest generalised entropy A(χB)/4GN + Sbulk(χB).”
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Self-citation
- Authors
- Hubeny, V. E., Rangamani, M., & Takayanagi, T.
- Affiliations
- Durham University (GB)
- Kyoto University (JP)
- ORCID
- Hubeny, Veronika E
- Venue
- Journal of High Energy Physics
- Published
- 2007-07-23
- Volume
- 2007
- Issue
- 07
- Pages
- 062-062
- ISSN
- 1029-8479 (ISSN-L)
- OpenAlex
- W2157692768
- Cited by
- 1,822
- References
- 50
- Citations by year
- 2026: 79 · 2025: 151 · 2024: 145 · 2023: 183 · 2022: 182 · 2021: 195 · 2020: 179 · 2019: 144 · 2018: 115 · 2017: 91 · 2016: 112 · 2015: 74 · 2014: 73 · 2013: 36 · 2012: 18
- FWCI
- 6.12
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Journal of High Energy Physics (publishedVersion)
- Durham Research Online (Durham University) (acceptedVersion)
- arXiv (Cornell University) (submittedVersion)
- Durham Research Online (Durham University) (submittedVersion, cc-by)
- arXiv (Cornell University)
- Funders
- Japan Society for the Promotion of Science (19GS0219)
- Kavli Institute for Theoretical Physics, University of California, Santa Barbara
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Quantum Electrodynamics and Casimir Effect
- Keywords
- holographic entanglement entropy, covariant entropy bound, light sheet, AdS/CFT correspondence, Euclidean wormholes
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