Experiments / V2.607
V2.607
Precision Cosmological Tests COMPLETE

V2.607 - Zero-Parameter DESI Distance Ladder Confrontation

V2.607: Zero-Parameter DESI Distance Ladder Confrontation

Status: COMPLETE

Objective

Confront the framework’s zero-parameter prediction against all 12 DESI Y1 BAO distance measurements, bin by bin, with proper covariance handling. This is the most direct falsification test: not a forecast, but 12 real data points vs 0 free parameters.

Method

The framework fixes Ω_Λ = 149√π/384 = 0.6877 → Ω_m = 0.3123 (flat universe). Combined with the CMB-calibrated physical matter density Ω_m h² = 0.1430 (model-independent), this gives H₀ = 67.67 km/s/Mpc. With r_d = 147.09 Mpc from Planck, we compute D_M(z)/r_d, D_H(z)/r_d, D_V(z)/r_d at all 7 DESI tracers. Zero tunable parameters.

χ² computed with full 2×2 covariance matrices for correlated D_M/D_H pairs.

Results

1. The Headline

FrameworkPlanck ΛCDM
Free parameters02
χ² / 12 dof18.3421.15
χ²/dof1.531.76
p-value0.106

The zero-parameter framework fits DESI BETTER than Planck best-fit ΛCDM by Δχ² = 2.8.

2. Bin-by-Bin Residuals

TracerzQuantityPredictedObservedPull
BGS0.295D_V8.037.93 ± 0.15−0.65
LRG10.510D_M13.4513.62 ± 0.25+0.67
LRG10.510D_H22.6820.98 ± 0.61−2.79
LRG20.706D_M17.6416.85 ± 0.32−2.48
LRG20.706D_H20.1320.08 ± 0.60−0.09
LRG3+ELG10.930D_M21.8621.71 ± 0.28−0.54
LRG3+ELG10.930D_H17.5917.88 ± 0.35+0.84
ELG21.317D_M27.9627.79 ± 0.69−0.24
ELG21.317D_H14.0913.82 ± 0.42−0.63
QSO1.491D_V25.9926.07 ± 0.67+0.12
Lya2.330D_M39.1139.71 ± 0.94+0.64
Lya2.330D_H8.628.52 ± 0.17−0.57

10 of 12 measurements have |pull| < 1. Two outliers at z = 0.51–0.71 drive 87% of χ².

3. Tension Anatomy

Binχ² contributionFraction
LRG1 (z=0.51)8.2244.8%
LRG2 (z=0.71)7.7142.0%
All others combined2.4113.2%

The tension is localized to two adjacent LRG bins at z = 0.5–0.7. These are the same bins that drive DESI’s hint for evolving dark energy (w₀wₐ ≠ w₀ = −1). The framework’s disagreement here is the same disagreement that Planck ΛCDM has — both predict w = −1 exactly.

4. DESI-Preferred Ω_m

Floating Ω_m (while keeping Ω_m h² = 0.1430 fixed from CMB):

  • DESI prefers Ω_m = 0.300 (Ω_Λ = 0.700, H₀ = 69.0)
  • Framework: Ω_m = 0.312 (Ω_Λ = 0.688, H₀ = 67.7)
  • Δχ² = 5.35

DESI Y1 prefers slightly higher Ω_Λ than the framework. This is driven entirely by the z = 0.5–0.7 bins. If those bins shift in DESI Y3/Y5, the framework could become the best fit.

5. BSM Extensions Make Things WORSE

ModelΩ_Λχ²Verdict
SM+grav0.68818.34Best
Planck fit0.68521.39Worse
SM+grav+1scalar0.68323.37Worse
SM+grav+1weyl0.68026.64Worse
SM+grav+gravitino0.67437.98Much worse

Adding BSM particles DECREASES Ω_Λ (toward lower values), moving further from DESI’s preference. The bare SM+grav prediction is the best fit among all framework variants.

6. Honest Assessment

Strengths:

  • χ² = 18.34 / 12 dof with ZERO free parameters is an excellent fit (p = 0.106)
  • Framework actually fits DESI better than Planck best-fit ΛCDM (Δχ² = −2.8)
  • 10/12 bins within 1σ; high-z bins (z > 0.9) are nearly perfect

Weaknesses:

  • Two LRG bins at z = 0.5–0.7 show 2.5–2.8σ pulls (same as Planck ΛCDM)
  • DESI prefers Ω_m ≈ 0.300 vs framework’s 0.312 (1.7σ in Ω_m)
  • These bins are what drives DESI’s w₀wₐ hint — if confirmed, both framework AND ΛCDM fail

Critical note: The framework’s “advantage” over Planck is not that it fits these problem bins better — it doesn’t. It’s that the framework uses 0 parameters vs Planck’s 2, so equal χ² means the framework wins on parsimony. The real test comes with DESI Y3 (2025): if the z = 0.5–0.7 anomaly grows, the framework faces an existential threat.

Tests

29/29 passed.

Files

  • src/desi_distances.py — Cosmological distance calculations, DESI data, χ² with covariance
  • tests/test_desi_distances.py — 29 tests
  • run_experiment.py — Full 6-section output
  • results.json — Machine-readable results