Pith. sign in
module module moderate

IndisputableMonolith.Cosmology.PhaseSaturationVacuum

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Defines the vacuum energy density parameter from phase saturation, tying the measured fine-structure constant to a closed-form Ω_Λ and proving elementary positivity and unit-interval bounds. Cosmologists comparing RS vacuum predictions to ΛCDM cite the bounds package. The argument is definitional plus short real-arithmetic inequalities from the external α anchor.

claimFix the measured fine-structure constant $\alpha>0$ as the sole external input. Define the phase-saturation vacuum density parameter $\Omega_\Lambda$ (in RS-native units) from $\alpha$, and establish $0 < \Omega_\Lambda < 1$ together with the seed comparison $\alpha/\pi < \Omega_\Lambda^{\mathrm{seed}}$ used downstream.

background

Recognition Science quarantines empirical calibration in ExternalAnchors so the cost-first core stays free of CODATA. This cosmology module imports that anchor for one measured quantity: the fine-structure constant $\alpha$, treated as a positive real seed rather than a derived RS constant.

The Cost and Constants layers supply the RS-native units and J-cost infrastructure; DimensionForcing records that spatial $D=3$ is already forced (T8), so the vacuum energy is interpreted in three-space. Phase saturation here means the residual vacuum density left after the recognition ledger closes on the $\phi$-ladder, expressed as a dimensionless density parameter $\Omega_\Lambda$ comparable to the ΛCDM dark-energy fraction.

Sibling lemmas package the elementary analytic facts: positivity of $\alpha$ and of $\alpha/\pi$, $\alpha<1/2$, and the corresponding positivity and upper bounds for $\Omega_\Lambda$.

proof idea

Definition module with a thin inequality layer. $\alpha$ is bound to the external measured anchor; $\Omega_\Lambda$ is introduced by a closed-form definition in terms of that anchor (and the RS unit conventions). Positivity and comparison lemmas are short real-arithmetic tactics: positivity of the seed, division by $\pi$, and the standard $0<x<1$ rearrangements that feed later Friedmann and phase-transition estimates. No deep forcing or RCL algebra appears here.

why it matters in Recognition Science

Feeds IndisputableMonolith.Cosmology.EWPhaseTransition, which builds the electroweak transition temperature and radiation-era Hubble rate on the $\phi$-ladder and needs a controlled vacuum density seed. Downstream status is explicitly MODEL (RS-native-unit scaffold): this module supplies the $\Omega_\Lambda$ bounds that keep that scaffold inside a physically admissible interval.

In the broader framework it sits after T8 ($D=3$) and the external $\alpha$ band (inverse fine structure near $137.03$–$137.04$), converting one measured input into a vacuum fraction usable by cosmology without reopening the forcing chain. It does not derive $\alpha$ from RCL; it only packages the saturation map and its elementary bounds.

scope and limits

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declarations in this module (42)