V2.85 Thermodynamic Uniqueness COMPLETE
KMS Equilibrium from Adiabatic FRW
Experiment V2.85: KMS Equilibrium from Adiabatic FRW
Status: COMPLETE
Goal
Show that standard QFT in curved spacetime (adiabatic vacuum) produces near-thermal horizons, establishing consistency with the equilibrium framework. Quantify the KMS deviation epsilon_KMS and derive the implied bound on N.
Key Results
| Background | epsilon_KMS (a=1) | epsilon_KMS (avg) |
|---|---|---|
| de Sitter | ~0 | ~0 |
| LCDM | 1.34e-02 | 3.54e-02 |
| Non-adiabatic | Large | Large |
- QFT-derived N bound: N <= 8.16e-02
- QFT consistency: YES (horizons are near-thermal)
The Chain of Logic
Standard QFT + Adiabatic Vacuum
|
Near-KMS Thermal Horizons (epsilon_KMS ~ 10^{-2})
|
Near-Clausius: delta_Q ~ T dS
|
Bounded d_iS: |d_iS| <= epsilon_KMS |dS|
|
QFT bound: N <= 0.1 <-- This experiment
+ Holographic/observational constraints
|
Full bound: N <= 10^{-3} <-- Requires additional arguments
Part A: KMS Deviation Measures
Defined two complementary measures of KMS deviation:
- Wightman-function KMS deviation (theoretical)
- Detector-response thermal deviation (operational)
Part B: Analytic Adiabatic Estimates
Derived the scaling relation: epsilon_KMS ~ O(|H_dot|/H^2, |H_dotdot|/H^3)
For slowly varying H(t):
- LCDM: epsilon_KMS << 1
- de Sitter: epsilon_KMS = 0 exactly
- Non-adiabatic: epsilon_KMS ~ O(1)
Part C: Unruh-DeWitt Detector Numerics
For LCDM:
- epsilon_KMS (max) = 4.24e-02
- epsilon_KMS (mean) = 2.86e-02
Part D: Connection to d_iS and N Bound
Established the key relation:
|d_iS| <= C_1 * epsilon_KMS * |dS_geo|
N <= C_1 * integral(epsilon_KMS(a) d ln a)
| Background | epsilon_KMS (avg) | N_bound | Threshold? |
|---|---|---|---|
| de Sitter | ~0 | ~0 | PASS |
| LCDM | 3.54e-02 | 8.16e-02 | PASS |
| Non-adiabatic | Large | Large | FAIL (expected) |
Important Caveat
QFT alone gives N <= 0.1, not N <= 10^{-3}. The tighter threshold comes from:
- Holographic arguments (V2.82 Part B): d_iS < 0.1% of horizon entropy
- Observational constraints (V2.79): Planck CMB constrains GR departures
- Jacobson’s derivation: horizons must be near-equilibrium for gravity to emerge
Modules
| Module | Purpose |
|---|---|
adiabatic_modes.py | Adiabatic mode functions |
frw_backgrounds.py | FRW background cosmologies |
kms_diagnostics.py | KMS deviation diagnostics |
thermo_bridge.py | Bridge to thermodynamic framework |
udw_detector.py | Unruh-DeWitt detector response |