Block 2: Cosmology
Modified Friedmann equations with the Λrel(z) correction that distinguishes the MCMC from the standard model.
ΛCDM vs MCMC
ΛCDM Model
Λ = constant
MCMC Model
Λ = Λ(z) dynamic
Indeterminate Channel ρ_id(z)
The density of the indeterminate channel (emergent dark energy) has a transitional behavior:
z > z_trans (High redshift)
Matter-like behavior: ρ ∝ (1+z)³
The indeterminate channel follows the dynamics of dark matter.
z ≤ z_trans (Low redshift)
Quasi-constant behavior
Transition to effective dark energy, modulated by ε.
Transition Parameters
| Parameter | Value | Description |
|---|---|---|
| z_trans | 8.9 ± 0.4 | Transition redshift |
| ε | 0.012 ± 0.003 | Transition coefficient |
| ρ₀ | 0.305 | Normalized base density |
Relative Lambda (Simplified Approximation)
For quick calculations, the MCMC correction can be approximated as:
This approximation with δΛ ≈ 0.02 captures the main behavior in the observable regime.
Correspondence with ΛCDM
The three primary components of the MCMC are mapped onto the parameters of standard cosmology:
Determinate Mass
Ω_b = 4.93%
Baryonic matterMCV (Latent)
Ω_DM = 26.6%
Dark matterECV (Indeterminate)
Ω_Λ = 68.5%
Dark energyMCMC Cosmological Parameters
| Parameter | Value | Prior Range | Description |
|---|---|---|---|
| H₀ | 69.6 ± 1.1 km/s/Mpc | [50, 100] | Hubble constant of the earlier corpus (production fits: 68.19 ± 0.40, with ΛCDM favored) |
| ρ_b0 | 0.0493 | [0.01, 1.0] | Normalized baryonic density |
| ρ₀ | 0.305 | [0.01, 2.0] | Base indeterminate density |
| z_trans | 8.9 ± 0.4 | [0.1, 3.0] | Transition redshift |
| ε | 0.012 ± 0.003 | [-0.5, 0.5] | Transition coefficient |
| r_d | 147 Mpc | [130, 160] | Sound horizon (BAO) |
| M | -19.4 mag | [-21, -18] | SNe Ia absolute magnitude |
H(z) Comparison: MCMC vs ΛCDM
Physical Interpretation
Why a Dynamic Λ?
In the MCMC, the cosmological constant is not really “constant.” It reflects the continuous process of conversion of mass into space:
- At high z (distant past): Λ_rel → 1 (ΛCDM recovered)
- At low z (present): Λ_rel slightly greater than 1
- The difference is small but measurable
Hubble Tension
The production fits run in August 2026 do not reproduce an alleviation of the Hubble tension: they give H₀ = 68.19 ± 0.40 km/s/Mpc and favor ΛCDM (ΔBIC +14.5). The current result is in the comparison.
Implementation in Python
📁 File: mcmc_core/bloque2_cosmologia.py