Experiments / V2.343
V2.343
Dynamical Selection COMPLETE

V2.343 - Framework vs w0waCDM — The DESI Confrontation

V2.343: Framework vs w0waCDM — The DESI Confrontation

Status: FRAMEWORK SURVIVES (BIC-preferred over w0waCDM with Bayes factor 8.3)

Objective

The framework predicts w = -1 exactly with ZERO free dark energy parameters. DESI (2024) hints at w0 != -1 (w0 ~ -0.85 in our fit). Does the DESI signal overcome the parameter penalty when comparing to the framework?

Method

Compared 4 models against 21 observations (CMB, DESI DR1 BAO, H0, SNe, growth):

ModelDE params (k)Description
Framework0Omega_L = 149*sqrt(pi)/384, w = -1 fixed
LCDM1Omega_L free, w = -1 fixed
w0CDM2Omega_L, w0 free, wa = 0
w0waCDM3Omega_L, w0, wa all free (CPL)

Model selection via AIC, BIC, and Bayes factors from BIC.

Key Results

Model comparison table

Modelkchi2AICBICDelta_BIC
Framework044.6344.6344.630.00
LCDM142.8944.8945.94+1.31
w0CDM240.5444.5446.63+2.00
w0waCDM339.7445.7448.87+4.24

Framework has the lowest BIC. Best by AIC is w0CDM (by 0.09, negligible).

Bayes factors (BIC approximation)

ComparisonBayes FactorInterpretation
Framework vs LCDM1.9Weak for framework
Framework vs w0CDM2.7Weak for framework
Framework vs w0waCDM8.3Substantial for framework
LCDM vs w0waCDM4.3Substantial for LCDM

w0 != -1 not significant

  • Delta_chi2(LCDM -> w0CDM) = 2.35 for 1 extra parameter (needs > 4.0)
  • Delta_chi2(LCDM -> w0waCDM) = 3.15 for 2 extra parameters (needs > 6.2)
  • Delta_chi2(Framework -> w0waCDM) = 4.89 for 3 extra parameters (needs > 8.0)

None of these improvements are statistically significant.

Best-fit w0waCDM parameters

  • w0 = -0.85, wa = -0.45, Omega_L = 0.689
  • Consistent with DESI 2024 findings but not significant over LCDM

Category chi2 breakdown

CategoryNFrameworkLCDMw0waCDM
CMB20.282.050.64
H021.841.191.62
BAO1218.2316.1313.51
SNe26.968.617.44
Growth317.3214.9116.53

Framework wins CMB and SNe categories; BAO drives the w0 != -1 preference (chi2 drops 18.23 -> 13.51 with 3 extra parameters), but the improvement is insufficient to overcome the BIC penalty.

What would kill the framework?

For w0waCDM to have lower BIC than framework:

  • Need chi2(w0waCDM) < 35.50
  • Currently: chi2(w0waCDM) = 39.74
  • Gap: 4.24 in chi2

If DESI DR3 halves BAO errors while maintaining w0 ~ -0.85:

  • Expected Delta_chi2 ~ 4x current ~ 20
  • This would exceed the 3*ln(21) = 9.1 BIC penalty
  • DESI DR3 is the decisive test

Significance

  1. The framework survives its biggest current threat. Despite DESI hints at evolving dark energy, the zero-parameter prediction w = -1, Omega_L = 0.6877 remains BIC-preferred.

  2. The parameter penalty is the framework’s shield. With k = 0 dark energy parameters, the framework gets no BIC penalty. w0waCDM must improve chi2 by > 9.1 to overcome its 3-parameter penalty.

  3. DESI DR3 will be decisive. If w0 ~ -0.85 persists with halved errors, the chi2 improvement will likely exceed the BIC threshold, killing the framework. If w0 returns to -1.0, the framework becomes even more strongly preferred.

Caveats

  1. Simplified likelihood: We use diagonal chi2 (no covariance matrices between BAO measurements at different redshifts).
  2. Limited data: 21 observations; full Planck + DESI analysis uses thousands of data points with full covariance.
  3. Nelder-Mead fits: Global optimality not guaranteed for w0waCDM, but results are consistent with DESI published values.

Files

  • src/w0wa_comparison.py: CosmoModel with CPL dark energy, fitting, model selection
  • run_experiment.py: 11-section analysis comparing 4 models
  • tests/test_w0wa.py: Unit tests (10 tests)