pith. machine review for the scientific record.
sign in

arxiv: 1911.11977 · v2 · pith:GKAYC3OKnew · submitted 2019-11-27 · ✦ hep-th · gr-qc· quant-ph

Replica wormholes and the black hole interior

Pith reviewed 2026-05-18 18:43 UTC · model grok-4.3

classification ✦ hep-th gr-qcquant-ph
keywords replica wormholesPage curveblack hole evaporationentanglement entropyholographyJT gravitySYK modelPetz map
0
0 comments X

The pith

Replica wormholes connecting different copies justify the holographic Page curve for black hole evaporation.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper shows that holographic calculations of the Page curve rely on the replica trick applied to the gravitational path integral. This requires summing over geometries that include spacetime wormholes linking the different replica systems. In a simple model the transition from linear growth to saturation in the radiation entropy arises when wormhole topologies dominate. The mechanism is checked in JT gravity with conformal matter and in the SYK model. A wormhole contribution also supplies a direct gravitational derivation of the Petz map for reconstructing the black hole interior from the radiation.

Core claim

Summing replica wormhole geometries in the gravitational path integral implements the replica trick for entanglement entropy. In a simple model, geometries with different numbers of wormholes produce the Page transition in the entropy of Hawking radiation. The same wormhole saddles appear in JT gravity coupled to matter and in the SYK model. The approach also yields an explicit gravitational formula for the Petz map that reconstructs the entanglement wedge of the black hole interior.

What carries the argument

Replica wormhole geometries in the gravitational path integral, which connect multiple replicas and whose inclusion and summation over topologies generates the correct Page curve for black hole radiation entropy.

If this is right

  • The entropy of the Hawking radiation follows the Page curve at late times.
  • The black hole interior is reconstructible from the radiation via the Petz map.
  • The gravity description implicitly averages over an ensemble of boundary theories.
  • Replica wormhole effects control entanglement calculations in both JT gravity and the SYK model.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The ensemble interpretation may link to questions about which boundary theory is dual to a given bulk geometry.
  • The same wormhole technique could be applied to other information-theoretic quantities in holographic models.
  • Replica wormholes might supply a general tool for computing late-time entanglement in systems with nontrivial topology.

Load-bearing premise

The gravitational path integral receives important non-perturbative contributions from replica wormhole geometries with connected topologies.

What would settle it

An explicit evaluation of the replica partition function that uses only disconnected geometries and fails to produce the Page transition in the simple model.

read the original abstract

Recent work has shown how to obtain the Page curve of an evaporating black hole from holographic computations of entanglement entropy. We show how these computations can be justified using the replica trick, from geometries with a spacetime wormhole connecting the different replicas. In a simple model, we study the Page transition in detail by summing replica geometries with different topologies. We compute related quantities in less detail in more complicated models, including JT gravity coupled to conformal matter and the SYK model. Separately, we give a direct gravitational argument for entanglement wedge reconstruction using an explicit formula known as the Petz map; again, a spacetime wormhole plays an important role. We discuss an interpretation of the wormhole geometries as part of some ensemble average implicit in the gravity description.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript claims that recent holographic computations of the Page curve for evaporating black holes can be justified using the replica trick applied to gravitational path integrals that include spacetime wormhole geometries connecting different replicas. In a simple model the authors sum over replica topologies with different connectivities to reproduce the Page transition explicitly. They sketch related calculations in JT gravity coupled to conformal matter and in the SYK model, give a direct gravitational derivation of entanglement-wedge reconstruction via the Petz map (again invoking a wormhole saddle), and discuss an ensemble-average interpretation of the wormhole contributions.

Significance. If the central claims hold, the work supplies a gravitational mechanism that derives the island formula and the Page curve from the replica trick, thereby addressing a key aspect of the black-hole information paradox within semiclassical gravity. The explicit topology summation performed in the simple model constitutes a concrete, falsifiable check of the proposed mechanism and is a clear strength of the manuscript.

major comments (2)
  1. [Section 3] Section 3: the replacement of the usual disconnected replica geometries by connected wormhole saddles is introduced as a postulate within an incompletely specified gravitational path integral; no UV completion or explicit measure is supplied that would justify why these non-perturbative saddles dominate and produce the Page transition. This assumption is load-bearing for the claimed justification of the island formula.
  2. [Discussion section] The ensemble-average interpretation of the wormhole geometries is presented as a plausible reading rather than a derived result; if this interpretation is intended to be part of the central claim, a more precise statement of what is derived versus conjectured is required.
minor comments (2)
  1. The notation for the replica index n and the on-shell actions of the various saddles could be standardized across sections to improve readability for readers outside the immediate subfield.
  2. A brief comparison table or figure summarizing the Page-transition behavior across the simple model, JT, and SYK would help readers assess the generality of the replica-wormhole mechanism.

Simulated Author's Rebuttal

2 responses · 1 unresolved

We thank the referee for their thoughtful review and for highlighting the strengths of our manuscript, including the explicit topology summation in the simple model. We address the major comments below and have revised the manuscript accordingly to improve clarity on the assumptions and interpretations.

read point-by-point responses
  1. Referee: [Section 3] Section 3: the replacement of the usual disconnected replica geometries by connected wormhole saddles is introduced as a postulate within an incompletely specified gravitational path integral; no UV completion or explicit measure is supplied that would justify why these non-perturbative saddles dominate and produce the Page transition. This assumption is load-bearing for the claimed justification of the island formula.

    Authors: We agree that the inclusion of connected wormhole saddles is a key assumption in our analysis of Section 3. The gravitational path integral is treated in a semiclassical approximation where we identify the relevant saddles, motivated by the replica trick and the need to reproduce the Page curve. While we do not provide a full UV completion, which remains an open question in quantum gravity, we explicitly demonstrate in the simple model how summing over replica topologies with wormholes leads to the Page transition. We have added text in the revised manuscript to more clearly state the assumptions underlying the path integral and to emphasize that our results are within the semiclassical regime. This should help clarify the justification for the island formula. revision: partial

  2. Referee: [Discussion section] The ensemble-average interpretation of the wormhole geometries is presented as a plausible reading rather than a derived result; if this interpretation is intended to be part of the central claim, a more precise statement of what is derived versus conjectured is required.

    Authors: We appreciate this point. The ensemble-average interpretation is indeed discussed as a possible way to understand the wormhole contributions in the context of the gravity description, but it is not central to our main claims about the replica trick justification and the Petz map. We have revised the discussion section to explicitly distinguish between the derived results from our calculations and the conjectural interpretation regarding ensemble averages. This includes a clearer statement that the main results hold independently of adopting this interpretation. revision: yes

standing simulated objections not resolved
  • A complete UV completion or explicit measure for the gravitational path integral that rigorously justifies the dominance of the non-perturbative wormhole saddles.

Circularity Check

0 steps flagged

No significant circularity; replica wormholes introduced as new saddles

full rationale

The paper applies the standard replica trick to gravitational path integrals and proposes connected wormhole geometries as additional non-perturbative saddles whose on-shell actions produce the Page transition. This step is not self-definitional, does not rename a fitted input as a prediction, and does not rest on a load-bearing self-citation whose content reduces to the present claim. The replica trick and holographic dictionary are invoked from prior literature as external tools, while the wormhole topologies are added as an independent assumption within the gravitational sum. No equation equates a derived quantity to an input parameter by construction, and the central result (island formula via replica wormholes) retains independent content beyond any cited works. The derivation is therefore self-contained against the paper's own stated assumptions.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The central claim rests on the standard holographic dictionary and the replica trick; the new element is the inclusion of connected wormhole saddles whose contribution is not derived from a more microscopic theory but is motivated by the need to reproduce the Page curve.

axioms (1)
  • domain assumption The gravitational path integral includes non-perturbative contributions from replica wormhole geometries.
    Invoked when the authors sum over topologies in the simple model to obtain the Page transition.

pith-pipeline@v0.9.0 · 5657 in / 1289 out tokens · 36041 ms · 2026-05-18T18:43:34.322916+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Forward citations

Cited by 20 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Wormholes and Averaging over N

    hep-th 2026-05 unverdicted novelty 8.0

    Mellin averaging over N reproduces the ensemble-like randomness of wormhole physics in the gravitational path integral when the dual theory admits analytic continuation in N and observables fluctuate superpolynomially...

  2. Replica Wormholes and the Entropy of Hawking Radiation

    hep-th 2019-11 accept novelty 8.0

    Replica wormholes in the gravitational path integral yield the island rule for the fine-grained entropy of Hawking radiation, ensuring it follows the unitary Page curve in two-dimensional dilaton gravity.

  3. Entanglement Wedge Reconstruction and the Information Paradox

    hep-th 2019-05 unverdicted novelty 8.0

    A phase transition in the quantum RT surface at the Page time derives the Page curve and enables entanglement wedge reconstruction of the black hole interior from Hawking radiation.

  4. Entanglement Revivals and Scrambling for Evaporating Black Holes

    hep-th 2026-04 unverdicted novelty 7.0

    Increasing black hole scrambling time in JT and RST evaporating geometries suppresses and eliminates late-time entanglement revivals in 2d CFT mutual information for disjoint intervals, interpolating between quasipart...

  5. Probing Evaporating Black Holes with Modular Flow in SYK

    hep-th 2025-12 unverdicted novelty 7.0

    Modular flow in SYK models coupled to a bath reveals singularities allowing reconstruction of bulk flow past the horizon in two-sided AdS2 black holes.

  6. Living on the edge: a non-perturbative resolution to the negativity of bulk entropies

    hep-th 2025-09 unverdicted novelty 7.0

    Summing non-perturbative contributions in the gravitational path integral, extended via matrix integral saddles including one- and two-eigenvalue instantons, resolves negativity of bulk entropies in two-sided black holes.

  7. Entanglement islands, fuzzballs and stretched horizons

    hep-th 2026-05 unverdicted novelty 6.0

    Fuzzball models with stretched horizons modify or eliminate entanglement islands depending on boundary conditions and cap geometry, producing information paradox analogues in some cases.

  8. Inner Horizon Saddles and a Spectral KSW Criterion

    hep-th 2026-05 unverdicted novelty 6.0

    Inner horizon saddles supply the semiclassical correction -exp(A_inner/4G) to near-extremal black-hole entropy and motivate a spectral KSW criterion for well-defined one-loop effects around complex gravitational saddles.

  9. Wormholes and the imaginary distance bound

    hep-th 2026-05 unverdicted novelty 6.0

    Wormhole effects in theories with imaginary massless scalars set an upper limit on analytic continuation of couplings to imaginary values, with string theory examples showing the low-energy theory breaks down at or be...

  10. Entanglement Revivals and Scrambling for Evaporating Black Holes

    hep-th 2026-04 unverdicted novelty 6.0

    Black hole scrambling suppresses and eventually eliminates late-time entanglement revivals in CFT mutual information for disjoint intervals, with spikes vanishing when interval lengths become exponential in the scramb...

  11. State counting in gravity and maximal entropy principle

    hep-th 2026-04 unverdicted novelty 6.0

    The Bekenstein-Hawking entropy state counting and the Page curve for Hawking radiation entanglement entropy are equivalent from the gravity path integral viewpoint via a convex optimization problem for von Neumann entropy.

  12. Probing the Factorized Island Branch with the Capacity of Entanglement in JT Gravity

    hep-th 2026-04 unverdicted novelty 6.0

    In JT gravity, the capacity of entanglement detects finite-n structure in the factorized island saddle that the entropy misses at first nontrivial order.

  13. Kerr Black Hole Ringdown in Effective Field Theory

    gr-qc 2026-03 unverdicted novelty 6.0

    Effective field theory yields model-independent corrections to Kerr black hole quasinormal modes that oscillate logarithmically near extremality, indicating discrete scale invariance.

  14. Menagerie of Euclidean constructions for 3D holographic cosmologies

    hep-th 2026-01 unverdicted novelty 6.0

    Generalized Euclidean wormhole constructions in 3D gravity produce holographic duals to approximately homogeneous closed baby-universe cosmologies and identify a necessary condition for the cosmological saddle to domi...

  15. Entanglement inequalities, black holes and the architecture of typical states

    hep-th 2025-11 unverdicted novelty 6.0

    Typical states in large-N holographic CFTs exhibit UV and IR length scales set by energy and charges, producing factorization that isolates black holes via a corona of saturated entanglement wedges and extends ETH to ...

  16. Single-Sided Black Holes in Double-Scaled SYK Model and No Man's Island

    hep-th 2025-11 unverdicted novelty 6.0

    In the double-scaled SYK model with an end-of-the-world brane, the boundary algebra for a single-sided black hole is a type II1 von Neumann factor with non-trivial commutant, preventing full bulk reconstruction and cr...

  17. How to have your wormholes and factorize, too

    hep-th 2026-02 unverdicted novelty 5.0

    A modified semiclassical holographic dictionary is used to construct an extended gravitational path integral that factorizes, reproduces the Page curve for entropy, and includes operators for baby universe states.

  18. Replica Phase Transition with Quantum Gravity Corrections

    hep-th 2026-02 unverdicted novelty 5.0

    The boundary theory of near-extremal RN black holes shows a replica phase transition controlled by temperature and the couplings C, K, and E.

  19. Quantum corrected black hole microstates and entropy

    hep-th 2025-09 unverdicted novelty 5.0

    In a doubly holographic black hole model, the dimension of the microstate Hilbert space equals the sum of the quantum-corrected thermodynamic entropies of the left and right black holes, which equals the generalised e...

  20. Gravitational Hilbert spaces: invariant and co-invariant states, inner products, gauge-fixing, and BRST

    hep-th 2025-09 unverdicted novelty 4.0

    Reviews construction of physical inner products in canonical quantum gravity via group averaging and BRST formalism, illustrated in mini-superspace models and connected to path integrals.

Reference graph

Works this paper leans on

101 extracted references · 101 canonical work pages · cited by 19 Pith papers · 58 internal anchors

  1. [1]

    Particle creation by black holes,

    S. W. Hawking, “Particle creation by black holes,” Comm. Math. Phys. 43 no. 3, (1975) 199–220. https://projecteuclid.org:443/euclid.cmp/1103899181

  2. [2]

    Average Entropy of a Subsystem

    D. N. Page, “Average entropy of a subsystem,” Phys. Rev. Lett. 71 (1993) 1291–1294, arXiv:gr-qc/9305007 [gr-qc]

  3. [3]

    Holographic Derivation of Entanglement Entropy from AdS/CFT

    S. Ryu and T. Takayanagi, “Holographic derivation of entanglement entropy from AdS/CFT,” Phys. Rev. Lett. 96 (2006) 181602, arXiv:hep-th/0603001 [hep-th]

  4. [4]

    A holographic proof of the strong subadditivity of entanglement entropy

    M. Headrick and T. Takayanagi, “A Holographic proof of the strong subadditivity of entanglement entropy,” Phys. Rev. D76 (2007) 106013, arXiv:0704.3719 [hep-th]

  5. [5]

    A Covariant Holographic Entanglement Entropy Proposal

    V. E. Hubeny, M. Rangamani, and T. Takayanagi, “A Covariant holographic entanglement entropy proposal,” JHEP 07 (2007) 062, arXiv:0705.0016 [hep-th]

  6. [6]

    Maximin Surfaces, and the Strong Subadditivity of the Covariant Holographic Entanglement Entropy

    A. C. Wall, “Maximin Surfaces, and the Strong Subadditivity of the Covariant Holographic Entanglement Entropy,” Class. Quant. Grav. 31 no. 22, (2014) 225007, arXiv:1211.3494 [hep-th]

  7. [7]

    Generalized gravitational entropy

    A. Lewkowycz and J. Maldacena, “Generalized gravitational entropy,” JHEP 08 (2013) 090, arXiv:1304.4926 [hep-th]

  8. [8]

    Quantum corrections to holographic entanglement entropy

    T. Faulkner, A. Lewkowycz, and J. Maldacena, “Quantum corrections to holographic entanglement entropy,” JHEP 11 (2013) 074, arXiv:1307.2892 [hep-th]

  9. [9]

    Deriving covariant holographic entanglement

    X. Dong, A. Lewkowycz, and M. Rangamani, “Deriving covariant holographic entanglement,” JHEP 11 (2016) 028, arXiv:1607.07506 [hep-th]

  10. [10]

    Holographic Entanglement Entropy

    M. Rangamani and T. Takayanagi, “Holographic Entanglement Entropy,” Lect. Notes Phys. 931 (2017) pp.1–246, arXiv:1609.01287 [hep-th]

  11. [11]

    Quantum Extremal Surfaces: Holographic Entanglement Entropy beyond the Classical Regime

    N. Engelhardt and A. C. Wall, “Quantum Extremal Surfaces: Holographic Entanglement Entropy beyond the Classical Regime,” JHEP 01 (2015) 073, arXiv:1408.3203 [hep-th]

  12. [12]

    Holographic Quantum Error Correction and the Projected Black Hole Interior

    A. Almheiri, “Holographic Quantum Error Correction and the Projected Black Hole Interior,” arXiv:1810.02055 [hep-th] . 74

  13. [13]

    Learning the Alpha-bits of Black Holes,

    P. Hayden and G. Penington, “Learning the Alpha-bits of Black Holes,” arXiv:1807.06041 [hep-th]

  14. [14]

    Entanglement Wedge Reconstruction and the Information Paradox

    G. Penington, “Entanglement Wedge Reconstruction and the Information Paradox,” arXiv:1905.08255 [hep-th]

  15. [15]

    The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole

    A. Almheiri, N. Engelhardt, D. Marolf, and H. Maxfield, “The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole,” arXiv:1905.08762 [hep-th]

  16. [16]

    The Page curve of Hawking radiation from semiclassical geometry

    A. Almheiri, R. Mahajan, J. Maldacena, and Y. Zhao, “The Page curve of Hawking radiation from semiclassical geometry,” arXiv:1908.10996 [hep-th]

  17. [17]

    Akers, N

    C. Akers, N. Engelhardt, and D. Harlow, “Simple holographic models of black hole evaporation,” arXiv:1910.00972 [hep-th]

  18. [18]

    Almheiri, R

    A. Almheiri, R. Mahajan, and J. Maldacena, “Islands outside the horizon,” arXiv:1910.11077 [hep-th]

  19. [19]

    Rozali, J

    M. Rozali, J. Sully, M. Van Raamsdonk, C. Waddell, and D. Wakeham, “Information radiation in BCFT models of black holes,” arXiv:1910.12836 [hep-th]

  20. [20]

    Information Flow in Black Hole Evaporation,

    H. Z. Chen, Z. Fisher, J. Hernandez, R. C. Myers, and S.-M. Ruan, “Information Flow in Black Hole Evaporation,” arXiv:1911.03402 [hep-th]

  21. [21]

    Bousso and M

    R. Bousso and M. Tomasevic, “Unitarity From a Smooth Horizon?,” arXiv:1911.06305 [hep-th]

  22. [22]

    Almheiri, R

    A. Almheiri, R. Mahajan, and J. E. Santos, “Entanglement islands in higher dimensions,” arXiv:1911.09666 [hep-th]

  23. [23]

    Entropy, Extremality, Euclidean Variations, and the Equations of Motion

    X. Dong and A. Lewkowycz, “Entropy, Extremality, Euclidean Variations, and the Equations of Motion,” JHEP 01 (2018) 081, arXiv:1705.08453 [hep-th]

  24. [24]

    A semiclassical ramp in SYK and in gravity

    P. Saad, S. H. Shenker, and D. Stanford, “A semiclassical ramp in SYK and in gravity,” arXiv:1806.06840 [hep-th]

  25. [25]

    JT gravity as a matrix integral

    P. Saad, S. H. Shenker, and D. Stanford, “JT gravity as a matrix integral,” arXiv:1903.11115 [hep-th]

  26. [26]

    Saad, Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity, 2019, [arXiv:1910.10311 [hep-th]]

    P. Saad, “Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity,” arXiv:1910.10311 [hep-th]

  27. [27]

    Eternal Black Holes in AdS

    J. M. Maldacena, “Eternal black holes in anti-de Sitter,” JHEP 04 (2003) 021, arXiv:hep-th/0106112 [hep-th]

  28. [28]

    The information paradox: A pedagogical introduction

    S. D. Mathur, “The Information paradox: A Pedagogical introduction,” Class. Quant. Grav. 26 (2009) 224001, arXiv:0909.1038 [hep-th]

  29. [29]

    Black Holes: Complementarity or Firewalls?

    A. Almheiri, D. Marolf, J. Polchinski, and J. Sully, “Black Holes: Complementarity or Firewalls?,” JHEP 02 (2013) 062, arXiv:1207.3123 [hep-th]

  30. [30]

    Complementarity Is Not Enough

    R. Bousso, “Complementarity Is Not Enough,” Phys. Rev. D87 no. 12, (2013) 124023, arXiv:1207.5192 [hep-th]

  31. [31]

    Complementarity Endures: No Firewall for an Infalling Observer

    Y. Nomura, J. Varela, and S. J. Weinberg, “Complementarity Endures: No Firewall for an Infalling Observer,” JHEP 03 (2013) 059, arXiv:1207.6626 [hep-th]

  32. [32]

    Black Hole Entanglement and Quantum Error Correction

    E. Verlinde and H. Verlinde, “Black Hole Entanglement and Quantum Error Correction,” JHEP 10 (2013) 107, arXiv:1211.6913 [hep-th]

  33. [33]

    An Infalling Observer in AdS/CFT

    K. Papadodimas and S. Raju, “An Infalling Observer in AdS/CFT,” JHEP 10 (2013) 212, arXiv:1211.6767 [hep-th]

  34. [34]

    Cool horizons for entangled black holes

    J. Maldacena and L. Susskind, “Cool horizons for entangled black holes,” Fortsch. Phys. 61 (2013) 781–811, arXiv:1306.0533 [hep-th]

  35. [35]

    Causality & holographic entanglement entropy

    M. Headrick, V. E. Hubeny, A. Lawrence, and M. Rangamani, “Causality & holographic entanglement entropy,” JHEP 12 (2014) 162, arXiv:1408.6300 [hep-th]

  36. [36]

    The Gravity Dual of a Density Matrix

    B. Czech, J. L. Karczmarek, F. Nogueira, and M. Van Raamsdonk, “The Gravity Dual of a Density Matrix,” Class. Quant. Grav. 29 (2012) 155009, arXiv:1204.1330 [hep-th]

  37. [37]

    Relative entropy equals bulk relative entropy

    D. L. Jafferis, A. Lewkowycz, J. Maldacena, and S. J. Suh, “Relative entropy equals bulk relative entropy,” JHEP 06 (2016) 004, arXiv:1512.06431 [hep-th] . 75

  38. [38]

    Reconstruction of Bulk Operators within the Entanglement Wedge in Gauge-Gravity Duality

    X. Dong, D. Harlow, and A. C. Wall, “Reconstruction of Bulk Operators within the Entanglement Wedge in Gauge-Gravity Duality,” Phys. Rev. Lett. 117 no. 2, (2016) 021601, arXiv:1601.05416 [hep-th]

  39. [39]

    Entanglement Wedge Reconstruction via Universal Recovery Channels,

    J. Cotler, P. Hayden, G. Penington, G. Salton, B. Swingle, and M. Walter, “Entanglement Wedge Reconstruction via Universal Recovery Channels,” Phys. Rev. X9 no. 3, (2019) 031011, arXiv:1704.05839 [hep-th]

  40. [40]

    Bulk locality from modular flow

    T. Faulkner and A. Lewkowycz, “Bulk locality from modular flow,” JHEP 07 (2017) 151, arXiv:1704.05464 [hep-th]

  41. [41]

    Sufficient subalgebras and the relative entropy of states of a von neumann algebra,

    D. Petz, “Sufficient subalgebras and the relative entropy of states of a von neumann algebra,” Communications in mathematical physics 105 no. 1, (1986) 123–131

  42. [42]

    Sufficiency of channels over von neumann algebras,

    D. Petz, “Sufficiency of channels over von neumann algebras,” The Quarterly Journal of Mathematics 39 no. 1, (1988) 97–108

  43. [43]

    Entanglement Wedge Reconstruction using the Petz Map,

    C.-F. Chen, G. Penington, and G. Salton, “Entanglement Wedge Reconstruction using the Petz Map,” JHEP 01 (2020) 168, arXiv:1902.02844 [hep-th]

  44. [44]

    Gravitation and Hamiltonian Structure in Two Space-Time Dimensions,

    C. Teitelboim, “Gravitation and Hamiltonian Structure in Two Space-Time Dimensions,” Phys. Lett. B126 (1983) 41–45

  45. [45]

    Lower Dimensional Gravity,

    R. Jackiw, “Lower Dimensional Gravity,” Nucl. Phys. B252 (1985) 343–356

  46. [46]

    Models of AdS_2 Backreaction and Holography

    A. Almheiri and J. Polchinski, “Models of AdS 2 backreaction and holography,” JHEP 11 (2015) 014, arXiv:1402.6334 [hep-th]

  47. [47]

    Black holes as mirrors: quantum information in random subsystems

    P. Hayden and J. Preskill, “Black holes as mirrors: Quantum information in random subsystems,” JHEP 09 (2007) 120, arXiv:0708.4025 [hep-th]

  48. [48]

    Two dimensional Nearly de Sitter gravity,

    J. Maldacena, G. J. Turiaci, and Z. Yang, “Two dimensional Nearly de Sitter gravity,” arXiv:1904.01911 [hep-th]

  49. [49]

    Replica Wormholes and the Entropy of Hawking Radiation

    A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian, and A. Tajdini, “Replica Wormholes and the Entropy of Hawking Radiation,” arXiv:1911.12333 [hep-th]

  50. [50]

    Pure states in the SYK model and nearly-$AdS_2$ gravity

    I. Kourkoulou and J. Maldacena, “Pure states in the SYK model and nearly- AdS2 gravity,” arXiv:1707.02325 [hep-th]

  51. [51]

    The Factorization Problem in Jackiw-Teitelboim Gravity,

    D. Harlow and D. Jafferis, “The Factorization Problem in Jackiw-Teitelboim Gravity,” arXiv:1804.01081 [hep-th]

  52. [52]

    Entanglement entropy in Jackiw-Teitelboim Gravity

    J. Lin, “Entanglement entropy in Jackiw-Teitelboim Gravity,” arXiv:1807.06575 [hep-th]

  53. [53]

    Entanglement Entropy in Jackiw-Teitelboim Gravity,

    D. L. Jafferis and D. K. Kolchmeyer, “Entanglement Entropy in Jackiw-Teitelboim Gravity,” arXiv:1911.10663 [hep-th]

  54. [54]

    Black Holes as Red Herrings: Topological Fluctuations and the Loss of Quantum Coherence,

    S. R. Coleman, “Black Holes as Red Herrings: Topological Fluctuations and the Loss of Quantum Coherence,” Nucl. Phys. B307 (1988) 867–882

  55. [55]

    Loss of Incoherence and Determination of Coupling Constants in Quantum Gravity,

    S. B. Giddings and A. Strominger, “Loss of Incoherence and Determination of Coupling Constants in Quantum Gravity,” Nucl. Phys. B307 (1988) 854–866

  56. [56]

    Free Probability Theory

    R. Speicher, “Free probability theory,” arXiv preprint arXiv:0911.0087 (2009)

  57. [57]

    PLANAR PERTURBATION EXPANSION,

    P. Cvitanovic, “PLANAR PERTURBATION EXPANSION,” Phys. Lett. 99B (1981) 49–52

  58. [58]

    The Quantum Gravity Dynamics of Near Extremal Black Holes,

    Z. Yang, “The Quantum Gravity Dynamics of Near Extremal Black Holes,” JHEP 05 (2019) 205, arXiv:1809.08647 [hep-th]

  59. [59]

    Statistical mechanics of a two-dimensional black hole

    A. Kitaev and S. J. Suh, “Statistical mechanics of a two-dimensional black hole,” JHEP 05 (2019) 198, arXiv:1808.07032 [hep-th]

  60. [60]

    Holographic Renyi Entropy from Quantum Error Correction

    C. Akers and P. Rath, “Holographic Renyi Entropy from Quantum Error Correction,” JHEP 05 (2019) 052, arXiv:1811.05171 [hep-th]

  61. [61]

    Flat entanglement spectra in fixed-area states of quantum gravity,

    X. Dong, D. Harlow, and D. Marolf, “Flat entanglement spectra in fixed-area states of quantum gravity,” JHEP 10 (2019) 240, arXiv:1811.05382 [hep-th] . 76

  62. [62]

    Structure of states which satisfy strong subadditivity of quantum entropy with equality,

    P. Hayden, R. Jozsa, D. Petz, and A. Winter, “Structure of states which satisfy strong subadditivity of quantum entropy with equality,” Communications in mathematical physics 246 no. 2, (2004) 359–374

  63. [63]

    Entanglement wedge reconstruction via universal recovery channels,

    J. Cotler, P. Hayden, G. Penington, G. Salton, B. Swingle, and M. Walter, “Entanglement wedge reconstruction via universal recovery channels,” Physical Review X 9 no. 3, (2019) 031011

  64. [64]

    Reversing quantum dynamics with near-optimal quantum and classical fidelity,

    H. Barnum and E. Knill, “Reversing quantum dynamics with near-optimal quantum and classical fidelity,” Journal of Mathematical Physics 43 no. 5, (2002) 2097–2106

  65. [65]

    Universal recovery maps and approximate sufficiency of quantum relative entropy,

    M. Junge, R. Renner, D. Sutter, M. M. Wilde, and A. Winter, “Universal recovery maps and approximate sufficiency of quantum relative entropy,” in Annales Henri Poincar´ e, vol. 19, pp. 2955–2978, Springer. 2018

  66. [66]

    Quantum Computation vs. Firewalls

    D. Harlow and P. Hayden, “Quantum Computation vs. Firewalls,” JHEP 06 (2013) 085, arXiv:1301.4504 [hep-th]

  67. [67]

    The Python’s Lunch: geometric obstructions to decoding Hawking radiation,

    A. R. Brown, H. Gharibyan, G. Penington, and L. Susskind, “The Python’s Lunch: geometric obstructions to decoding Hawking radiation,” arXiv:1912.00228 [hep-th]

  68. [68]

    Entanglement entropy and conformal field theory

    P. Calabrese and J. Cardy, “Entanglement entropy and conformal field theory,” J. Phys. A42 (2009) 504005, arXiv:0905.4013 [cond-mat.stat-mech]

  69. [69]

    Gapless Spin-Fluid Ground State in a Random Quantum Heisenberg Magnet

    S. Sachdev and J.-w. Ye, “Gapless spin fluid ground state in a random, quantum Heisenberg magnet,” Phys. Rev. Lett. 70 (1993) 3339, arXiv:cond-mat/9212030 [cond-mat]

  70. [70]

    A simple model of quantum holography talk1 and talk2

    A. Kitaev, “A simple model of quantum holography talk1 and talk2.”. Talks at KITP, April 7, 2015 and May 27, 2015

  71. [71]

    The soft mode in the Sachdev-Ye-Kitaev model and its gravity dual

    A. Kitaev and S. J. Suh, “The soft mode in the Sachdev-Ye-Kitaev model and its gravity dual,” JHEP 05 (2018) 183, arXiv:1711.08467 [hep-th]

  72. [72]

    Spread of entanglement in a Sachdev-Ye-Kitaev chain

    Y. Gu, A. Lucas, and X.-L. Qi, “Spread of entanglement in a Sachdev-Ye-Kitaev chain,” JHEP 09 (2017) 120, arXiv:1708.00871 [hep-th]

  73. [73]

    Wave function of the universe,

    J. B. Hartle and S. W. Hawking, “Wave function of the universe,” Phys. Rev. D 28 (Dec, 1983) 2960–2975. https://link.aps.org/doi/10.1103/PhysRevD.28.2960

  74. [74]

    Density matrix of the universe,

    D. N. Page, “Density matrix of the universe,” Phys. Rev. D 34 (Oct, 1986) 2267–2271. https://link.aps.org/doi/10.1103/PhysRevD.34.2267

  75. [75]

    Density matrix of the Universe reloaded: origin of inflation and cosmological acceleration

    A. Barvinsky, C. Deffayet, and A. Y. Kamenshchik, “Density matrix of the universe reloaded: origin of inflation and cosmological acceleration,” arXiv preprint arXiv:0810.5659 (2008)

  76. [76]

    A simple model of quantum holography slides here,

    J. Maldacena, “A simple model of quantum holography slides here,.”. Talks at Strings 2019

  77. [77]

    Low-dimensional de Sitter quantum gravity,

    J. Cotler, K. Jensen, and A. Maloney, “Low-dimensional de Sitter quantum gravity,” arXiv:1905.03780 [hep-th]

  78. [78]

    Non-gaussian features of primordial fluctuations in single field inflationary models,

    J. Maldacena, “Non-gaussian features of primordial fluctuations in single field inflationary models,” Journal of High Energy Physics 2003 no. 05, (May, 2003) 013013. http://dx.doi.org/10.1088/1126-6708/2003/05/013

  79. [79]

    Higher Spin Realization of the dS/CFT Correspondence

    D. Anninos, T. Hartman, and A. Strominger, “Higher Spin Realization of the dS/CFT Correspondence,” Class. Quant. Grav. 34 no. 1, (2017) 015009, arXiv:1108.5735 [hep-th]

  80. [80]

    Cosmological event horizons, thermodynamics, and particle creation,

    G. W. Gibbons and S. W. Hawking, “Cosmological event horizons, thermodynamics, and particle creation,” Phys. Rev. D 15 (May, 1977) 2738–2751. https://link.aps.org/doi/10.1103/PhysRevD.15.2738

Showing first 80 references.