Generalized Entropy and Quantum Extremal Surfaces
Generalized entropy combines matter entropy with geometric entropy terms in a common renormalized prescription. It connects horizon thermodynamics to quantum extremal surfaces, while distinguishing stationarity, monotonicity, and entropy-reconstruction claims.
Enter this chapter
Section titled “Enter this chapter”Begin with Black-Hole Thermodynamics at the QFT Interface to separate horizon temperature, flux, and entropy as physical quantities.
Helpful background. Replica Trick and Branched Geometries and Entropy Counterterms and Renormalization Ambiguities develop the definitions used by the chapter’s opening pages.
Topics
Section titled “Topics”- Black-Hole Thermodynamics at the QFT Interface — Separates Hawking temperature, state-dependent flux, and geometric entropy.
- Fine-Grained, Coarse-Grained, and Algebraic Entropy — Fixes the entropy object before calculations begin.
- Horizon Entanglement Entropy — Derives the local ultraviolet structure across a smooth horizon.
- Relative Entropy and Modular Horizon Laws — Develops finite algebraic comparisons and known modular generators.
- Generalized Entropy and UV Renormalization — Combines matter and gravitational counterterms.
- Species, Gauge Edges, and Contact Terms — Makes the algebra and edge prescription explicit.
- Noether-Charge Entropy and Higher-Curvature Terms — Derives stationary geometric entropy from the action.
- Replica Constructions on Fixed and Semiclassical Backgrounds — States the boundary, saddle, symmetry, and continuation assumptions.
- Conical Entropy and Effective-Action Variations — Tracks bulk, surface, and contact contributions.
- Semiclassical First Laws and Physical-Process Variations — Distinguishes equilibrium variation from flux-driven change.
- The Generalized Second Law: Hypotheses and Proven Scope — States precisely which causal-horizon results are proved.
- Quantum Extremal Surfaces: Renormalized Semiclassical Definition — Defines renormalized stationarity and perturbative displacement.
- Semiclassical Black-Hole Information: Scope and Limits — Identifies what evaporation arguments require beyond this chapter.
How the ideas fit together
Section titled “How the ideas fit together”The ultraviolet dependence of matter entanglement must be combined with the renormalization of gravitational surface terms. Once that generalized entropy is defined, varying the surface gives the quantum-extremality condition Engelhardt and Wall 2015, §§ 2–3.
Stationarity identifies candidate surfaces; it does not by itself select a dominant saddle or prove a boundary entropy formula. The generalized second law instead concerns monotonicity under stated horizon and state assumptions. Keeping these questions separate prevents a local entropy variation from being mistaken for a complete black-hole information calculation.
The comparison below separates the assumptions and tests needed for these different conclusions.
Domain and failure conditions
Section titled “Domain and failure conditions”| Object or statement | State and algebra | Regulator and geometry | Licensed conclusion | Status | Failure or further method needed |
|---|---|---|---|---|---|
| Hawking thermodynamics | Declared black-hole state; exterior observables | Stationary nonextremal Killing horizon; renormalized stress tensor | , flux after greybody scattering, stationary first-law data | QFT calculation plus classical geometry | A rapidly evolving trapping horizon lacks the required symmetry |
| Fine/coarse entropy | State on an algebra; coarse constraints specified | UV regulator only for subregion entropy | Distinguish von Neumann, relative, and thermodynamic entropy | Definition/algebraic theorem | Type-III local algebras defeat naive tensor-factor entropy arithmetic |
| Horizon entanglement | Hadamard-like short-distance state; chosen algebra | Smooth cut; explicit UV regulator | Local area and curvature divergences; finite differences when controlled | QFT calculation | Regulator-dependent constants are not observables |
| Relative/modular law | Normal states on one algebra; modular domains valid | Often regulator free | Positivity, monotonicity, near a reference state | Operator-algebra theorem | A geometric is unavailable for a generic region/state |
| Renormalized | Matter state and algebra fixed | Matter and gravitational counterterms matched | Finite scheme-consistent generalized-entropy differences/variations | Semiclassical EFT construction | Shifting only one sector produces spurious scheme dependence |
| Gauge/edge entropy | Center or edge prescription declared | Gauge-compatible regulator and contact terms | Comparable entropy within that prescription | Algebra-dependent construction | Changing the algebra while holding counterterms fixed changes the question |
| Noether-charge entropy | Classical stationary solution | Diffeomorphism-invariant renormalized action; bifurcate Killing surface | Wald entropy and stationary first law | Classical theorem/semiclassical coupling input | Dynamical cuts carry ambiguity and extra flux terms |
| Replica entropy | State preparation and replica boundary data | Integer covers; action, defects, and saddles specified | if continuation exists | Path-integral calculation | Integer data need not select the derivative at |
| Conical effective action | Matter boundary conditions and zero modes fixed | Smoothed cone or distributional prescription | Bulk/surface/contact contribution to entropy | One-loop calculation | Cone and UV limits may not commute |
| First law | Perturbation of a stationary reference state | Linear order; suitable horizon and asymptotics | Equality among charge, flux, area, and modular variations | Perturbative theorem | Shear, expansion, and quadratic entropy production matter beyond linear order |
| Generalized second law | Horizon algebra and regular state satisfy stated axioms | Causal horizon; joint renormalization; semiclassical regime | Monotonic for the theorem’s slices | Theorem in specified field classes | Apparent horizons and generic interacting theories are not automatic corollaries |
| Quantum extremal surface | and declared | Admissible anchored/homologous surface class; renormalized functional | and controlled displacement | Semiclassical definition/calculation | Stationarity alone neither minimizes nor supplies an island formula |
| Information claim | Exterior/radiation algebra and operational task fixed | Evaporation approximation and gravity input stated | A scoped entropy or recovery statement | Model-dependent/open | Mean Hawking flux alone cannot establish a Page curve or microscopic unitarity |
Where to go next
Section titled “Where to go next”Continue to Energy Conditions, Inequalities, and Focusing to identify which classical energy condition a quantum expectation value violates.
References
Section titled “References”- Engelhardt, N., and A. C. Wall, “Quantum Extremal Surfaces: Holographic Entanglement Entropy beyond the Classical Regime,” Journal of High Energy Physics 2015, 073 (2015), doi:10.1007/JHEP01(2015)073.