Keyboard shortcuts

Press or to navigate between chapters

Press S or / to search in the book

Press ? to show this help

Press Esc to hide this help

Generalized Entropy: Unification of Geometry and Quantum

“Entropy comes not only from matter, but also from spacetime itself.”

🎯 Core Question

In the Foundation chapter, we learned Boltzmann entropy:

But in the presence of gravity, this definition is incomplete!

Why?

Because spacetime itself carries entropy!

🌟 Revelation of Bekenstein-Hawking Entropy

Black Hole Entropy

In 1973, Bekenstein proposed: black holes should have entropy.

In 1974, Hawking calculated:

Where:

  • : horizon area
  • : Newton’s gravitational constant
  • : Planck constant

Key observations:

  1. Entropy is proportional to area, not volume!
  2. Entropy contains gravitational constant
  3. Entropy contains quantum constant

This means: Entropy is the intersection of gravity, quantum, and thermodynamics!

graph TB
    BH["Black Hole Entropy<br/>S_BH = A/4Gℏ"]

    BH --> G["Gravity<br/>G"]
    BH --> Q["Quantum<br/>ℏ"]
    BH --> T["Thermodynamics<br/>k_B"]
    BH --> GEO["Geometry<br/>Area A"]

    style BH fill:#fff4e1,stroke:#ff6b6b,stroke-width:3px
    style G fill:#e1f5ff
    style Q fill:#e1ffe1
    style T fill:#ffe1e1
    style GEO fill:#f5e1ff

📐 Definition of Generalized Entropy

Sum of Two Terms

In quantum gravity, generalized entropy is defined as:

Where:

  • : spatial hypersurface (Cauchy slice)
  • : area of boundary of
  • : von Neumann entropy of quantum fields outside the boundary

Physical Meaning

graph TB
    subgraph "Spatial Hypersurface Σ"
        B["Boundary ∂Σ<br/>Area A"]
    end

    subgraph "Outside Region"
        O["Quantum Field State ρ<br/>Entropy S_out = -tr(ρ ln ρ)"]
    end

    S["Generalized Entropy<br/>S_gen"] --> G["Geometric Contribution<br/>A/4Gℏ"]
    S --> Q["Quantum Contribution<br/>S_out"]

    B -.-> G
    O -.-> Q

    style S fill:#fff4e1,stroke:#ff6b6b,stroke-width:3px
    style G fill:#e1f5ff
    style Q fill:#ffe1e1

First term (geometric entropy):

  • From degrees of freedom of spacetime geometry
  • Same form as black hole entropy
  • Reflects “gravitational entropy” of boundary

Second term (quantum field entropy):

  • From quantum entanglement of matter fields
  • von Neumann entropy:
  • Reflects “information entropy” of fields

💡 Balloon Analogy

Imagine a balloon:

🎈

Total “information” = information on balloon surface + information of internal gas

AnalogyPhysics
Balloon surface areaBoundary area
Surface wrinkles, textureGeometric entropy
Internal gas moleculesQuantum fields
Gas entropyField entropy
Total informationGeneralized entropy

Key insight:

We cannot only look at the gas (matter fields), but also the balloon itself (spacetime geometry)!

🔬 Generalized Entropy on Small Causal Diamond

In the IGVP framework, we define generalized entropy on the small causal diamond .

Structure of Small Causal Diamond

graph TB
    Q["Future Vertex<br/>q"] --> |"Past Null Cone"| W["Waist S_ℓ<br/>Boundary of Maximum Spatial Cross-Section"]
    P["Past Vertex<br/>p"] --> |"Future Null Cone"| W

    W --> A["Area A(S_ℓ)"]
    W --> V["Volume V(B_ℓ)"]

    style W fill:#fff4e1,stroke:#ff6b6b,stroke-width:2px
    style Q fill:#ffe1e1
    style P fill:#e1f5ff

Waist :

  • Boundary of maximum spatial cross-section in the diamond
  • Dimension: ( is spacetime dimension)
  • Area:

Volume :

  • Volume of maximum spatial cross-section
  • Volume:

Explicit Form of Generalized Entropy

On the small causal diamond:

Meaning of each term:

  1. : geometric entropy of waist
  2. : renormalized field entropy
  3. : UV counterterm (handles divergence)
  4. : volume dual term (Lagrange multiplier)

Temperature :

Where is the surface gravity of the approximate Killing field.

🌊 Why Renormalization?

Divergence Problem

In quantum field theory, entanglement entropy diverges at short distances:

( is UV cutoff)

Solution:

  1. Point-splitting renormalization: Use fine regularization scheme
  2. Subtract divergent terms:
  3. Keep finite part: is finite as

Physical Meaning of Renormalization

graph LR
    R["Raw Field Entropy<br/>S_out^raw"] --> |"Subtract UV Divergence"| C["Counterterm<br/>S_ct^UV"]
    R --> |"Subtract"| REN["Renormalized Entropy<br/>S_out^ren"]
    C -.-> REN

    style R fill:#ffe1e1
    style C fill:#f0f0f0,stroke-dasharray: 5 5
    style REN fill:#e1ffe1

Physical interpretation:

  • UV divergent terms are absorbed by geometric term
  • Finite part is physical
  • This is similar to mass renormalization

📊 Properties of Generalized Entropy

Property 1: Monotonicity

During evolution, generalized entropy is considered to satisfy the second law:

Along affine parameter of null geodesics.

This suggests the existence of a thermodynamic arrow of time.

Property 2: Extremality

On solutions of Einstein’s equations, generalized entropy takes an extremum at the waist of the small causal diamond:

This is the first-order variational condition of IGVP.

Property 3: Concavity

Second-order variation is typically non-negative:

This provides a theoretical guarantee for the stability of solutions.

🔗 Connection to Core Insights

Entropy is the Arrow

Monotonicity of generalized entropy defines the arrow of time:

Boundary is Reality

Geometric entropy term emphasizes the ontological status of boundary area.

Time is Geometry

Temperature connects thermal time with geometric time.

📝 Key Formulas Summary

FormulaNameMeaning
Bekenstein-Hawking entropyBlack hole entropy
Generalized entropyGeometry + quantum
von Neumann entropyQuantum field entropy
Unruh temperatureTemperature of accelerated observer

🎓 Further Reading

  • Original paper: J.D. Bekenstein, “Black holes and entropy” (Phys. Rev. D 7, 2333, 1973)
  • Hawking radiation: S.W. Hawking, “Black hole explosions?” (Nature 248, 30, 1974)
  • Generalized entropy: T. Faulkner et al., “Gravitation from entanglement” (JHEP 03, 051, 2014)
  • GLS documentation: igvp-einstein-complete.md
  • Next: 02-causal-diamond_en.md - Small Causal Diamond

🤔 Exercises

  1. Conceptual understanding:

    • Why is black hole entropy proportional to area rather than volume?
    • What physical degrees of freedom do the two terms of generalized entropy come from?
    • Why is renormalization needed?
  2. Order-of-magnitude estimates:

    • What is the horizon area of a solar-mass black hole? What is the Bekenstein-Hawking entropy?
    • How does it compare with the thermodynamic entropy of gas inside the Sun?
  3. Physical applications:

    • How does Hawking radiation maintain monotonicity of generalized entropy?
    • How does the Page curve reflect evolution of generalized entropy?
    • What is the relationship between black hole information paradox and generalized entropy?
  4. Advanced thinking:

    • What problems would arise if the geometric entropy term is not included?
    • How does Wald entropy (higher-order gravity theories) generalize ?
    • What is the connection between holographic entanglement entropy and generalized entropy?

Next step: After understanding generalized entropy, we will learn where it is varied—the small causal diamond!