Encyclopedia Cosmology Cosmology Dark Energy Evolution Structure Dark Energy Implies Ne One

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Cosmology Dark Energy Evolution Structure Dark Energy Implies Ne One

A formal result pins dark energy's density to a narrow band: positive, but strictly less than the whole universe.

The dark energy bound

Dark energy is the name cosmologists give to the unknown agent that accelerates the expansion of the universe. Its density is usually written as ΩΛ, the fraction of the universe's total energy budget that behaves like a cosmological constant. In the standard picture, that fraction sits near 0.7, and observations place it firmly between zero and one.

The Recognition Science framework addresses a narrower question: what bounds follow from its own structural assumptions. The framework models the universe's history as a ledger, a discrete record of recognition events, and derives a cosmological constant resolution from that picture. Within this account, a theorem named dark_energy_implies_ne_one shows that the dark energy density cannot equal 1, and a companion theorem shows it cannot equal 0 either. Together with the positivity bound, the framework proves that 0 < ΩΛ < 1.

The result is a formal consequence of the framework's own definitions, checked in its machine-checked library of formal theorems. It does not tell us what the value of ΩΛ actually is, only that it lies strictly inside the open interval from zero to one. The theorem rules out the two degenerate endpoints: a universe with no dark energy at all, and a universe made entirely of dark energy.

What the declaration does not claim is just as important. It does not assert that dark energy evolves over time, despite the name of the surrounding file. The framework's current formal content establishes a bound, not a time-dependent equation of state. It also does not predict a numerical value for ΩΛ, and it does not engage with the measured value from supernova surveys or cosmic microwave background data. Those comparisons remain outside this particular formal result.

THEOREM omega_lambda_bounded · dark_energy_evolution_structure · IndisputableMonolith/Cosmology/DarkEnergyEvolutionStructure.lean
/-- Baseline RS dark-energy density is positive and subunitary. -/
theorem omega_lambda_bounded :
    0 < EarlyUniverse.omega_lambda ∧ EarlyUniverse.omega_lambda < 1 :=
  EarlyUniverse.cosmological_constant_resolution
theorem dark_energy_evolution_structure : dark_energy_evolution_from_ledger := omega_lambda_bounded
THEOREM dark_energy_implies_ne_zero · dark_energy_implies_ne_one · IndisputableMonolith/Cosmology/DarkEnergyEvolutionStructure.lean
/-- Dark-energy structure excludes the degenerate `Ω_Λ = 0` endpoint. -/
theorem dark_energy_implies_ne_zero (h : dark_energy_evolution_from_ledger) :
    EarlyUniverse.omega_lambda ≠ 0 :=
  ne_of_gt h.1
/-- Dark-energy structure excludes the degenerate `Ω_Λ = 1` endpoint. -/
theorem dark_energy_implies_ne_one (h : dark_energy_evolution_from_ledger) :
    EarlyUniverse.omega_lambda ≠ 1 :=
  ne_of_lt h.2

What this page does not claim

The declaration does not assert that dark energy evolves over time. The declaration does not predict a numerical value for Ω<sub>Λ</sub>. The declaration does not compare against measured cosmological data.

Verify this page

Every tagged claim above names its theorem. To check one yourself rather than trust this page, elaborate the source module with Lean 4 and audit its axiom basis:

$ lake env lean IndisputableMonolith/Cosmology/DarkEnergyEvolutionStructure.lean
expected axiom basis: [propext, Classical.choice, Quot.sound] (the Lean kernel's standard three; no RS-specific axioms)

A page whose claims cannot be reproduced this way does not ship. In production, every anchor links to the exact declaration in the public source release, and this block carries the build receipt for the page itself.

Derived articles

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