Encyclopedia Cosmology Cosmology Dark Energy Equation Of State W Lambda
Cosmology Dark Energy Equation Of State W Lambda
In cosmology, the dark energy equation of state w measures how dark energy responds to expansion; the value -1 is the cosmological constant baseline.
A baseline and its bound
In cosmology, the equation of state parameter w for dark energy is the ratio of its pressure to its energy density. A value of w = -1 corresponds to the cosmological constant, the simplest model where dark energy has a fixed density in space. This baseline is what the Recognition Science declaration wLambda establishes: it defines the baseline value as exactly -1.
The framework's library also defines a correction bound, bitCorrectionBound, equal to phi - 3/2, where phi is the golden ratio. This evaluates to approximately 0.118. The library states that the absolute deviation of w from -1, written |w - (-1)|, is bounded by this value. This bound is presented as an exact closed form, not an approximation, because of the identity 1/phi = phi - 1.
In Recognition Science, the framework models dark energy through its own internal structure. Its prediction is that the present-day value w_0 lies in the interval (-1 - J(phi), -1), approximately (-1.13, -1), where J(phi) is the same golden-ratio-based constant. This means the framework predicts a phantom-like dark energy, with w_0 less than -1, but bounded away from the baseline by no more than about 0.118.
The declaration itself is a definition, not a measurement. It sets the baseline for the framework's own cosmological model. The bound is a separate definition, and the prediction is a hypothesis stated in the documentation, not a proved theorem in the library. The library contains no proof that the actual observed value of w satisfies this bound; it only defines the bound and the baseline.
MODEL wLambda · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- Dark energy EoS w_0 = -1 (cosmological constant baseline). -/
def wLambda : ℝ := -1
MODEL bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- BIT correction bound: `|δw| ≤ J(φ)`. This is the exact phantom-Carnot ceiling
`J(φ) = φ − 3/2 ≈ 0.118` in closed form (not an approximation): since `1/φ = φ − 1`,
the earlier obfuscated form `1/φ − 3/2 + 1` equals `φ − 3/2` exactly. -/
noncomputable def bitCorrectionBound : ℝ := phi - 3 / 2
MODEL bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- BIT correction bound: `|δw| ≤ J(φ)`. This is the exact phantom-Carnot ceiling
`J(φ) = φ − 3/2 ≈ 0.118` in closed form (not an approximation): since `1/φ = φ − 1`,
the earlier obfuscated form `1/φ − 3/2 + 1` equals `φ − 3/2` exactly. -/
noncomputable def bitCorrectionBound : ℝ := phi - 3 / 2
What this page does not claim
The declaration does not prove any observed value of w satisfies the bound. The framework does not claim to derive the cosmological constant from first principles. The prediction of w_0 in the interval (-1.13, -1) is a hypothesis, not a proved theorem.
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/DarkEnergyEquationOfState.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
This page is generated by a question-recursion engine: the questions its answers raise become the next pages. The current agenda, with open targets marked red:
- What physical mechanism in the framework produces the phantom-like prediction w_0 < -1?
- How does the framework's bound on w relate to observational constraints from supernovae and cosmic microwave background data?
- What is the status of the prediction that w_0 lies in the interval (-1.13, -1) as a formal theorem in the library?
MACHINE LAYER · GROUNDED CLAIM TABLE · CLICK TO EXPAND
MODEL wLambda · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- Dark energy EoS w_0 = -1 (cosmological constant baseline). -/ def wLambda : ℝ := -1The Recognition Science declaration wLambda defines the baseline value as exactly -1. wLambda · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.leanMODEL bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- BIT correction bound: `|δw| ≤ J(φ)`. This is the exact phantom-Carnot ceiling `J(φ) = φ − 3/2 ≈ 0.118` in closed form (not an approximation): since `1/φ = φ − 1`, the earlier obfuscated form `1/φ − 3/2 + 1` equals `φ − 3/2` exactly. -/ noncomputable def bitCorrectionBound : ℝ := phi - 3 / 2The library defines a correction bound, bitCorrectionBound, equal to phi - 3/2, which evaluates to approximately 0.118. bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.leanMODEL bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean
/-- BIT correction bound: `|δw| ≤ J(φ)`. This is the exact phantom-Carnot ceiling `J(φ) = φ − 3/2 ≈ 0.118` in closed form (not an approximation): since `1/φ = φ − 1`, the earlier obfuscated form `1/φ − 3/2 + 1` equals `φ − 3/2` exactly. -/ noncomputable def bitCorrectionBound : ℝ := phi - 3 / 2The library states that the absolute deviation of w from -1 is bounded by this value. bitCorrectionBound · IndisputableMonolith/Cosmology/DarkEnergyEquationOfState.lean