IndisputableMonolith.Cosmology.DarkEnergyEvolutionStructure
The module structures dark energy evolution in Recognition Science, establishing that baseline density is positive and subunitary. Cosmologists working on the small cosmological constant within the RS framework would cite it to connect early-universe ledger conditions to late-time acceleration. It imports the EarlyUniverse module and organizes the relevant structural results.
claimBaseline RS dark-energy density $\rho_{\rm DE}$ satisfies $0 < \rho_{\rm DE} < 1$.
background
The module belongs to the Cosmology domain and imports IndisputableMonolith.Cosmology.EarlyUniverse. That upstream module formalizes the RS derivation of early universe conditions and dark energy, covering registry items EU-001 (Big Bang at t=0), D-002 (what is dark energy), and D-003 (why the cosmological constant is small). The supplied doc-comment states the central property: baseline RS dark-energy density is positive and subunitary.
proof idea
This is a definition module, no proofs.
why it matters in Recognition Science
The module supplies the evolution structure that supports resolution of D-002 and D-003 in the EarlyUniverse module. It ensures the density remains positive and subunitary, feeding the RS account of the small cosmological constant.
scope and limits
- Does not derive the numerical value of the cosmological constant.
- Does not model explicit time-dependent evolution equations.
- Does not incorporate observational data from supernovae or CMB.