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IndisputableMonolith.Cosmology.DarkEnergy

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The Cosmology.DarkEnergy module defines the present-day Hubble parameter H₀ ≈ 2.2 × 10^{-18} s^{-1} together with Planck time, universe age, cosmic ratios, spacetime regions, balance conditions, densities, expansion tension, and the cosmological constant in RS-native units. It extends the Constants and Cost modules to cosmological scales for expansion and dark energy work. The module consists entirely of definitions with no theorems or proofs.

claim$H_0 ≈ 2.2 \times 10^{-18} \, \mathrm{s}^{-1}$ (today's Hubble parameter), $t_{\mathrm{planck}}$, $t_{\mathrm{universe}}$, cosmic ratio, SpacetimeRegion, isBalanced, entryDensity, costDensity, expansionTension, cosmologicalConstant, and $\Lambda > 0$.

background

The module imports IndisputableMonolith.Constants, whose doc states the fundamental RS time quantum τ₀ = 1 tick, and IndisputableMonolith.Cost. It introduces sibling definitions H0, t_planck, t_universe, cosmicRatio, cosmic_ratio_large, SpacetimeRegion, isBalanced, entryDensity, costDensity, expansionTension, cosmologicalConstant, and lambda_positive. These objects operate in the cosmology domain and apply the core RS time quantum and cost structures at large scales.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

The module supplies the Hubble parameter and cosmological constant that support dark energy and expansion modeling in the Recognition Science framework. It connects the Constants and Cost modules to cosmological applications, enabling density and tension calculations. No downstream theorems are recorded in the dependency graph.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (27)