Encyclopedia Gravity Gravity Full Efewith Dark Energy Flat Vacuum Stress Conserved

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Gravity Full Efewith Dark Energy Flat Vacuum Stress Conserved

In general relativity, a cosmological constant does not disturb the equations of motion. A machine-checked proof now shows why this holds in a flat spacetime model.

The conserved vacuum

In Einstein's general relativity, the stress-energy tensor describes the density and flow of energy and momentum in spacetime. The Bianchi identity, a geometric fact about the curvature of spacetime, implies that this tensor is covariantly conserved: its covariant derivative vanishes. This conservation is not an extra assumption; it is a necessary consequence of the field equations. A cosmological constant, often denoted Λ, represents a constant energy density of empty space, and it is incorporated into the field equations as an additional term proportional to the metric tensor.

The declaration flat_vacuum_stress_conserved, a theorem in the Recognition Science framework's machine-checked library, proves a specific instance of this conservation. It establishes that for a flat spacetime, the Minkowski metric, and a vacuum stress-energy tensor that is a constant multiple of that metric, the covariant derivative is identically zero. The proof relies on two key facts: the metric is covariantly constant (metric compatibility), and the covariant derivative is linear with respect to scalar multiplication. The theorem states that for any constant c, the covariant derivative of c times the metric is zero. This is the structural reason a cosmological constant is always consistent with the conservation law.

This result is part of a larger effort to integrate a dark energy term into the framework's Einstein field equations. The framework defines a specific positive cosmological constant, Λ_RS, and shows that the extended field equations recover the baseline when the Hubble parameter squared goes to zero. The vacuum equation of state is exactly w = -1, meaning the pressure is the negative of the energy density. The theorem flat_vacuum_stress_conserved provides the necessary consistency check for this term in a flat reference spacetime.

What the theorem does not claim is that the cosmological constant is conserved in a general, curved spacetime. The proof is specific to the flat Minkowski metric and a particular choice of connection. It does not establish the value of the cosmological constant, nor does it prove that dark energy exists. It only shows that a particular mathematical construction, a constant times the metric, is consistent with the conservation law in the flat case. The physical recognition-to-linking bridge that would connect this to a broader theory of quantum gravity remains an open target.

THEOREM flat_vacuum_stress_conserved · IndisputableMonolith/Gravity/FullEFEWithDarkEnergy.lean
/-- **VACUUM TERM IS COVARIANTLY CONSERVED (flat reference, grounded).** Specialization of
`vacuum_stress_conserved` to the flat reference, using the proved
`minkowski_metric_compatible`. No metric compatibility is assumed; it is discharged. -/
theorem flat_vacuum_stress_conserved (c : ℝ) :
    ∀ lam mu nu : Connection.Idx,
      covDeriv02 (Connection.christoffel_from_metric Connection.minkowski_inverse (fun _ _ _ => 0))
        (fun a b => c * Connection.minkowski.g a b) (fun a b d => c * (fun _ _ _ => (0 : ℝ)) a b d)
        lam mu nu = 0 :=
  vacuum_stress_conserved c Connection.minkowski
    (Connection.christoffel_from_metric Connection.minkowski_inverse (fun _ _ _ => 0))
    (fun _ _ _ => 0) minkowski_metric_compatible
THEOREM minkowski_metric_compatible · covDeriv02_smul · IndisputableMonolith/Gravity/FullEFEWithDarkEnergy.lean
/-- The flat Minkowski metric is covariantly constant: `∇_λ g_μν = 0`. Both the ordinary
derivative (constant metric) and the Christoffel symbols (flat) vanish. -/
theorem minkowski_metric_compatible :
    Connection.metric_compatibility Connection.minkowski
      (Connection.christoffel_from_metric Connection.minkowski_inverse (fun _ _ _ => 0))
      (fun _ _ _ => 0) := by
  unfold Connection.metric_compatibility
  intro lam mu nu
  simp [Connection.flat_christoffel_vanish]
/-- Linearity of the (0,2) covariant derivative: scaling the tensor (and its ordinary
derivative) by a constant `c` scales the covariant derivative by `c`. -/
theorem covDeriv02_smul (ch : Connection.ChristoffelData)
    (Tg : Connection.Idx → Connection.Idx → ℝ)
    (dT : Connection.Idx → Connection.Idx → Connection.Idx → ℝ)
    (c : ℝ) (lam mu nu : Connection.Idx) :
    covDeriv02 ch (fun a b => c * Tg a b) (fun a b d => c * dT a b d) lam mu nu
      = c * covDeriv02 ch Tg dT lam mu nu := by
  have hs1 : ∑ rho : Connection.Idx, (ch.gamma rho lam mu * (c * Tg rho nu))
           = c * ∑ rho : Connection.Idx, (ch.gamma rho lam mu * Tg rho nu) := by
    rw [Finset.mul_sum]; apply Finset.sum_congr rfl; intro rho _; ring
  have hs2 : ∑ rho : Connection.Idx, (ch.gamma rho lam nu * (c * Tg mu rho))
           = c * ∑ rho : Connection.Idx, (ch.gamma rho lam nu * Tg mu rho) := by
    rw [Finset.mul_sum]; apply Finset.sum_congr rfl; intro rho _; ring
  simp only [covDeriv02]
  rw [hs1, hs2]; ring
THEOREM Lambda_RS_pos · recovers_baseline_lambda · IndisputableMonolith/Gravity/FullEFEWithDarkEnergy.lean
/-- `Λ_RS` is positive for any positive Hubble scale (forced by `Ω_Λ > 0`). -/
theorem Lambda_RS_pos {H0sq : ℝ} (h : 0 < H0sq) : 0 < Lambda_RS H0sq := by
  unfold Lambda_RS
  exact mul_pos (mul_pos (by norm_num : (0 : ℝ) < 3) h) Omega_Lambda_RS_pos
/-- The Λ-extended data recovers the baseline `Λ = 0` data in the limit. -/
theorem recovers_baseline_lambda :
    (rs_efe_data_with_lambda 0).cosmological_constant
      = FullEFE.rs_efe_data.cosmological_constant := by
  show Lambda_RS 0 = 0
  exact Lambda_RS_zero
THEOREM vacuum_eos · IndisputableMonolith/Gravity/FullEFEWithDarkEnergy.lean
/-- **VACUUM EQUATION OF STATE IS `w = −1`.** The static vacuum fluid has `p/ρ = −1`. -/
theorem vacuum_eos (rho : ℝ) (h : rho ≠ 0) : vacuum_pressure rho / rho = -1 := by
  unfold vacuum_pressure
  rw [neg_div, div_self h]

What this page does not claim

The theorem does not prove conservation in a general curved spacetime. The theorem does not establish the existence or value of the cosmological constant. The theorem does not connect the flat spacetime result to a physical theory of quantum gravity.

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/Gravity/FullEFEWithDarkEnergy.lean
expected axiom basis: [propext, Classical.choice, Quot.sound] (the Lean kernel's standard three; no RS-specific axioms)

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