V2.141 - Effective Dark Energy Equation of State from Horizon Thermodynamics
V2.141: Effective Dark Energy Equation of State from Horizon Thermodynamics
Status: COMPLETE
Question
V2.138 found 3.3-4.2 sigma DESI tension against w = -1. The framework predicts Lambda is constant. But the Clausius relation is applied at the apparent horizon, which CHANGES in LCDM (the universe is not exactly de Sitter). Does the time-evolving horizon produce an effective w(z) that deviates from -1? And is Lambda stable through the electroweak phase transition?
Method
Two analyses:
A) Non-equilibrium correction: Apply the Clausius relation at the evolving LCDM apparent horizon r_A = c/H(z). As the horizon area A(z) = 4pi/E^2(z) changes with redshift, the log correction S_log = delta * ln(A) also changes. Does this source an effective w != -1?
B) Phase transition stability: At the electroweak transition (~100 GeV), the field content changes: 4 massless gauge bosons + 4 scalars -> 1 massless + 3 massive vectors + 1 scalar (Goldstone bosons eaten). Does this change R = |delta|/(6*alpha)?
Results
Phase 1: LCDM Background
The apparent horizon shrinks dramatically at higher redshift:
| z | H(z) km/s/Mpc | q(z) | r_A (Hubble units) |
|---|---|---|---|
| 0 | 67.36 | -0.527 | 1.000 |
| 1 | 120.66 | +0.180 | 0.558 |
| 2 | 204.37 | +0.389 | 0.330 |
| 3 | 307.85 | +0.451 | 0.219 |
The transition from deceleration (q > 0) to acceleration (q < 0) occurs at z ~ 0.6.
Phase 2: Naive w(z) — the WRONG Answer
If one naively applies the self-consistency condition at each redshift, treating Lambda(z) ∝ E^2(z), the effective equation of state is:
| z | w_naive |
|---|---|
| 0 | -0.685 |
| 0.5 | -0.391 |
| 1.0 | -0.213 |
| 2.0 | -0.074 |
This gives huge deviations from w = -1. But this is WRONG. The self-consistency condition determines Lambda at the de Sitter ENDPOINT (z -> -1), not at each intermediate redshift. At finite z, the Clausius relation generates the full Friedmann equation with Lambda as a CONSTANT.
Phase 3: Correct w(z) — Non-equilibrium Correction
The correct treatment fixes Lambda at the de Sitter equilibrium. Non-equilibrium corrections from entropy production are second-order in deviations from de Sitter and suppressed by l_P^2/r_A^2 ~ 10^{-122}:
| z | w(z) | |w + 1| | |---|------|---------| | 0 | -1.000… | 7.8 x 10^{-124} | | 0.5 | -1.000… | 5.1 x 10^{-123} | | 1.0 | -1.000… | 1.6 x 10^{-122} | | 2.0 | -1.000… | 6.2 x 10^{-122} |
Maximum |w + 1| = 1.5 x 10^{-121}, utterly undetectable.
The suppression has a clear physical origin:
- Non-equilibrium entropy production is quadratic in deviations: ~(H_dot/H^2)^2
- The ratio of log to area corrections provides the factor: |delta|/(alpha * A/l_P^2) ~ 10^{-122}
- Combined: |w + 1| ~ Omega_m^2 * delta/(alpha * 10^{122}) ~ 10^{-122}
Phase 4: DESI Comparison
The framework predicts w = -1 exactly (to 10^{-120}). Against DESI:
| Dataset | w0 | wa | Tension |
|---|---|---|---|
| DR2 + PantheonPlus | -0.752 | -1.01 | 4.2 sigma |
| DR2 + DESY5 | -0.775 | -0.84 | 3.3 sigma |
| DR1 + PantheonPlus | -0.827 | -0.75 | 2.0 sigma |
Phase 5: Electroweak Phase Transition Stability
Symmetric phase (T >> 100 GeV): 12 massless vectors + 4 scalars + 45 Weyls
- alpha_eff = 118, delta = -1991/180
Broken phase (T << 100 GeV): 9 massless + 3 massive vectors + 1 scalar + 45 Weyls
- alpha_eff = 118, delta = -1991/180
Both alpha and delta are IDENTICAL. The Goldstone equivalence theorem guarantees this: the 3 eaten Goldstone bosons become the longitudinal polarizations of W+, W-, Z. A massive Proca field = massless vector + scalar in terms of both alpha (heat kernel tr(1)) and delta (trace anomaly). So R = |delta|/(6*alpha) is exactly preserved.
Lambda is EXACTLY constant through the electroweak transition.
Key Findings
-
w = -1 to ~10^{-120} precision. Non-equilibrium corrections from the evolving LCDM horizon are suppressed by l_P^2/r_A^2 ~ 10^{-122}. The framework has NO mechanism to produce w != -1 at any detectable level.
-
Lambda is exactly stable through EWSB. The Goldstone equivalence theorem ensures alpha and delta are identical in symmetric and broken phases. R is exactly preserved.
-
Three independent upper bounds on |w + 1| from the framework:
- Mass corrections: |w+1| < 10^{-32} (V2.130)
- Non-equilibrium: |w+1| < 10^{-121} (this experiment)
- Phase transitions: |w+1| = 0 exactly (this experiment)
-
DESI tension: up to 4.2 sigma. This is the framework’s most serious current challenge. If DESI confirms w != -1 at > 5 sigma, the framework is FALSIFIED. This is a genuine, sharp, falsifiable prediction.
Implications
The framework makes an extraordinarily rigid prediction: w = -1 with no room for deviation. There are no free parameters that can be adjusted, no higher-order corrections that can help, and no phase transition effects that could produce time-dependent dark energy.
This rigidity is both a strength (sharp falsifiability) and a vulnerability (no escape route if DESI w != -1 is confirmed). The framework essentially predicts that DESI’s evidence for dynamical dark energy will not survive to 5 sigma as more data accumulates.
Files
run_experiment.py: 6-phase experiment driversrc/horizon_thermodynamics.py: LCDM cosmology, horizon entropy, w(z) computationssrc/phase_transition.py: EW phase transition stability analysistests/test_horizon_thermo.py: 17 tests (all pass)results/results.json: Full numerical data
References
- Cai & Kim (2005): First law at apparent horizon
- Akbar & Cai (2006): Friedmann equation from first law
- Jacobson (1995, 2016): Thermodynamic gravity
- DESI DR2 (2025): Evidence for dynamical dark energy