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Key Findings (v0.1.0)

This page states what the final Protocol 1b run supports, in the order result → interpretation → caveat. The data are 1,590 Pantheon+SH0ES supernovae and 13 DESI DR2 BAO measurements, sampled with 100,000 steps and 96 walkers per model.

ProtocolProtocol 1b — Pantheon+SH0ES + DESI DR2 BAO
Data1,590 SNe (z > 0.01) + 13 BAO · N = 1,603
Sampleremcee · 100,000 steps × 96 walkers · burn-in 20,000
Fixedr_d = 147.09 Mpc
Statusv0.1.0 exploratory
Exploratory

None of the findings below is a detection. Each is conditional on a fixed sound horizon, bounded priors and a fixed reference cosmology for the Ξosc time axis (Known Limitations).


Key results​

18.3
ΔAIC of ΛCDM
vs CPL (lowest AIC) · N = 1,603
1.94
ΔAIC of Ξosc
vs CPL · χ² lowest: Ξosc
0.185
Oscillation amplitude ε
+0.077 −0.087 · prior 0 < ε < 0.3
2.26σ
ε / σ_ε (symmetrised)
descriptive ratio, not a detection

1. ΛCDM is disfavoured by this dataset combination​

Result. ΛCDM has ΔAIC = 18.3 relative to the best model, with χ² = 1554.2 against 1531.8 for CPL and 1529.8 for Ξosc.

Interpretation. Both dynamical models fit the combined data markedly better than a constant w = −1 does, even after the AIC penalty for their extra parameters. This suggests that the data prefer something other than w = −1 within this setup — it does not identify which.

Caveat. The BIC, which penalises parameters more heavily, narrows the gap (next section), and r_d is fixed rather than marginalised.

2. CPL and Ξosc are close by AIC; the BIC reorders the three​

Modelχ²kAICBICΔAIC
CPL1531.82441539.8241561.3430.000
Ξosc1529.76361541.7631574.0411.939
ΛCDM1554.16521558.1651568.92418.341

Result. CPL has the lowest AIC and the lowest BIC. Ξosc has the lowest raw χ² but ΔAIC = 1.94 relative to CPL. Under the BIC, Ξosc (1574.041) falls behind ΛCDM (1568.924).

Interpretation. The extra two parameters of Ξosc buy a small χ² gain that the AIC almost forgives and the BIC does not. The data do not single out the oscillating model.

Caveat. The χ² of each model is the best sampled point of its chain, not an exact minimum; see Model Comparison.

3. A non-zero amplitude is allowed, but it is prior-limited​

Result. ε = 0.185 (+0.077, −0.087), i.e. ε/σε ≈ 2.26 with a symmetrised σε.

Interpretation. The posterior prefers ε > 0, but ε is sampled under a one-sided prior (0 < ε < 0.3), and the corner plot shows its distribution rising towards the upper bound. The ratio is a descriptive summary; it is not the significance of a detection.

Caveat. T and φ₀ remain weakly constrained. Details: Ξosc Oscillation Diagnostic.

4. The final chains satisfy the practical convergence criterion​

Result. N/50 = 2,000 exceeds the largest autocorrelation time of Ξosc, τmax = 1504 (parameter T).

Caveat. The criterion measures sampling noise, not prior-boundary pile-up or multimodality. See Convergence Diagnostics.


Evidence level​

These statements correspond to the ξ entries of the Claims Register: preliminary for the amplitude preference, and not stronger for anything else.