Encyclopedia Cosmology Cosmology Dark Energy Eos Constant Energy Contribution
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Cosmology Dark Energy Eos Constant Energy Contribution
In cosmology, dark energy is often modeled as a constant energy density filling space. Recognition Science proves that such a constant contribution must have an equation of state parameter of exactly -1.
A constant energy contribution
In standard cosmology, dark energy is the name for whatever is causing the accelerated expansion of the universe. The simplest model treats it as a constant energy density, a fixed amount of energy in every cubic centimeter of space that does not dilute as the universe expands. The key question is how the pressure of this energy relates to its density, a ratio written as w. For an ordinary gas, w is positive. For dark energy, observations point to w being very close to -1, meaning the energy exerts a kind of negative pressure, a suction that drives the expansion faster.
The mathematical object called a constant energy contribution in the Recognition Science framework is a precise way of stating this idea. It is defined as a structure with three parts: a positive real number for the energy density, a proof that this number is greater than zero, and a condition that the energy does not depend on time. The framework then defines the equation of state parameter as the negative of the energy density divided by itself, which simplifies to -1. A theorem in the framework's machine-checked library of formal theorems proves this result: for any such constant energy contribution, the equation of state parameter is exactly -1.
The physical reasoning behind the theorem is the relativistic condition for a vacuum. In general relativity, a Lorentz-invariant vacuum has a stress-energy tensor proportional to the metric, which forces the pressure to be the negative of the energy density. The framework's contribution is to derive this condition from its own ledger picture, where a phase-locked mode has a committed record at a ratio of 1, and its recognition cost is zero at every tick. The energy of such a mode is constant across space and time, so it behaves as a constant energy density and therefore has w = -1.
What the declaration does not claim is that this constant energy density is the actual dark energy in our universe. It proves a conditional statement: if you have a constant energy contribution, then its equation of state is -1. It does not prove that such a contribution exists in nature, nor does it derive the measured value of the dark energy density. The framework also does not claim that w is exactly -1 for all possible dark energy models; it only applies to the specific case of a constant energy density, not to models where the energy changes with time or space.
THEOREM w_eq_neg_one · IndisputableMonolith/Cosmology/DarkEnergyEOS.lean
/-- **THEOREM (w = -1)**: A constant energy density has w = -1.
Proof: w = p/ρ. For a Lorentz-invariant constant energy density,
the stress-energy tensor is T_μν = -ρ·g_μν (proportional to the
metric). Therefore p = -ρ and w = p/ρ = -ρ/ρ = -1.
In the ledger picture: phase-locked modes have J(1) = 0 at every
tick. Their energy is the mode energy E_coh/16, which is the same
at every lattice site (translation symmetry) and at every tick
(phase locking). A spatially uniform, temporally constant energy
density in GR has w = -1 identically. -/
theorem w_eq_neg_one (c : ConstantEnergyContribution) :
equation_of_state c = -1 := by
unfold equation_of_state
rw [neg_div, div_self (ne_of_gt c.energy_pos)]
MODEL ConstantEnergyContribution · IndisputableMonolith/Cosmology/DarkEnergyEOS.lean
/-- Energy density of a constant (tick-independent) contribution.
A contribution whose energy doesn't change with volume satisfies
the thermodynamic relation dE = -p dV.
If E is constant: dE = 0 = -p dV, so either p = 0 (trivial) or
we need the relativistic form: ρ + p = 0 for a Lorentz-invariant
vacuum, giving p = -ρ and w = p/ρ = -1. -/
structure ConstantEnergyContribution where
energy_density : ℝ
energy_pos : 0 < energy_density
tick_independent : True
What this page does not claim
The declaration does not prove that a constant energy contribution exists in nature. The declaration does not derive the measured value of the dark energy density. The declaration does not apply to dark energy models with a time-varying equation of state.
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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:
- How does the framework derive the existence of a constant energy contribution from its ledger picture?
- What physical mechanism in the framework sets the numerical value of the dark energy density?
- Does the framework's derivation of w = -1 apply to dark energy models with a time-varying equation of state?
- How does the framework's phase-locked mode relate to the standard quantum field theory vacuum?
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THEOREM w_eq_neg_one · IndisputableMonolith/Cosmology/DarkEnergyEOS.lean
/-- **THEOREM (w = -1)**: A constant energy density has w = -1. Proof: w = p/ρ. For a Lorentz-invariant constant energy density, the stress-energy tensor is T_μν = -ρ·g_μν (proportional to the metric). Therefore p = -ρ and w = p/ρ = -ρ/ρ = -1. In the ledger picture: phase-locked modes have J(1) = 0 at every tick. Their energy is the mode energy E_coh/16, which is the same at every lattice site (translation symmetry) and at every tick (phase locking). A spatially uniform, temporally constant energy density in GR has w = -1 identically. -/ theorem w_eq_neg_one (c : ConstantEnergyContribution) : equation_of_state c = -1 := by unfold equation_of_state rw [neg_div, div_self (ne_of_gt c.energy_pos)]A theorem in the framework's machine-checked library proves that for any constant energy contribution, the equation of state parameter is exactly -1. w_eq_neg_one · IndisputableMonolith/Cosmology/DarkEnergyEOS.leanMODEL ConstantEnergyContribution · IndisputableMonolith/Cosmology/DarkEnergyEOS.lean
/-- Energy density of a constant (tick-independent) contribution. A contribution whose energy doesn't change with volume satisfies the thermodynamic relation dE = -p dV. If E is constant: dE = 0 = -p dV, so either p = 0 (trivial) or we need the relativistic form: ρ + p = 0 for a Lorentz-invariant vacuum, giving p = -ρ and w = p/ρ = -1. -/ structure ConstantEnergyContribution where energy_density : ℝ energy_pos : 0 < energy_density tick_independent : TrueA constant energy contribution is defined as a structure with a positive energy density and a condition that the energy does not depend on time. ConstantEnergyContribution · IndisputableMonolith/Cosmology/DarkEnergyEOS.lean