We test the hypothesis that the expansion history of the universe can be described not by the standard ΛCDM model, but by a power-law scaling of the form a(t) ∝ t^α or even a dynamically evolving exponent α(t) modeled within a scalar–tensor framework.
-
Type Ia Supernovae (Pantheon+SH0ES)
https://pantheonplussh0es.github.io/ -
Gamma-Ray Bursts (GRB)
Calibrated from Amati relation, see arXiv:1610.00854 -
Cosmic Chronometers (CC)
Hubble parameter from differential galaxy ages, see arXiv:2009.10701 -
Planck 2018 CMB TT Power Spectrum
Transformed into log-distance-like domain for joint likelihood fitting, see esdcdoi.esac.esa.int
| Dataset | Model | H₀ | α or Ωₘ | χ² | AIC | BIC |
|---|---|---|---|---|---|---|
| CC | ΛCDM | 68.16 | 0.319 | 14.55 | 18.55 | 21.49 |
| Time-Scaling | 70.00 | 1.252 | 25.17 | 29.17 | 32.11 | |
| SN | ΛCDM | 71.42 | 0.351 | 758.58 | 762.58 | 773.46 |
| Time-Scaling | 70.89 | 1.388 | 763.42 | 767.42 | 778.30 | |
| GRB | ΛCDM | 75.00 | 0.500 | 167.36 | 171.36 | 177.53 |
| Time-Scaling | 75.00 | 1.000 | 174.97 | 178.97 | 185.15 | |
| CMB | ΛCDM | 67.19 | — | 84136.8 | 84138.8 | 84144.6 |
| Time-Scaling | 70.00 | 1.966 | 83939.5 | 83943.5 | 83955.1 | |
| Combined | ΛCDM | 65.00 | 0.357 | 626542.7 | 626550.7 | 626576.3 |
| Time-Scaling | 70.00 | 1.060 | 225288.4 | 225296.4 | 225321.9 |
ΔAIC = 401254.37 → Strong evidence in favor of Time-Scaling model in the global fit.
We model α(t) as a scalar field coupled to gravity via a Brans–Dicke–like action, and test three potentials:
- Quadratic: V(α) ∝ α²
- Cosine: V(α) ∝ cos(α)
- Asymmetric: V(α) ∝ α³·sin(α)
Key finding: time-directionality emerges under asymmetric potentials — Lyapunov analysis shows:
- Forward evolution: λₗ ~ 10⁻³
- Backward evolution: λₗ < 0
No thermodynamic or quantum mechanisms are required to induce the arrow of time.
.
├── model.py # Full numerical analysis pipeline
├── results.txt # Full fitting + MCMC + dynamics output
├── fig_obs.png # Fits to SN, GRB, CC, and CMB
├── fig_obs_combined.png # Combined observational fit
├── fig_dynamics.png # Scalar field evolution (α(t))
├── fig_lyap.png # Lyapunov exponent analysis
├── fig_mcmc.png # Posterior samples for ΛCDM and Time-Scaling
└── README.md # This file
Having Python ≥ 3.10, install dependencies:
pip install numpy scipy matplotlib pandas sympy emceepython model.pyOutputs include:
- Full observational fitting (SN, GRB, CC, CMB)
- Global AIC/BIC comparison
- Posterior sampling (optional MCMC)
- Scalar dynamics and Lyapunov evolution
- All plots saved as PNG
If using this code or results, please cite:
Chudzik, A. (2025). Revisiting the relationship between the scale factor a(t) and cosmic time t using numerical analysis. Mathematics (MDPI).