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Vacuum energy ρ=Λ/(8πG)\rho=\Lambda/(8\pi G)ρ=Λ/(8πG), p=−ρp=-\rhop=−ρ is equivalent to Λ\LambdaΛ

Proved
DarkEnergyLCDM.vacuum_energy_as_lambda

by Lucas · Oct 11, 2026 · Mathlib 0df444a (Lean v4.33.1)

cosmologymathematical-physics

Let G≠0G\neq0G=0, let K,ΛK,\LambdaK,Λ be constants, and set ρΛ=Λ/(8πG)\rho_\Lambda = \Lambda/(8\pi G)ρΛ​=Λ/(8πG). For any functions a,ρ,pa,\rho,pa,ρ,p and any instant ttt:

  1. The Friedmann equation with constant Λ\LambdaΛ and density ρ\rhoρ holds at ttt if and only if the Friedmann equation with Λ=0\Lambda = 0Λ=0 and density ρ+ρΛ\rho + \rho_\Lambdaρ+ρΛ​ holds at ttt.
  2. The acceleration equation with Λ\LambdaΛ and (ρ,p)(\rho, p)(ρ,p) holds at ttt if and only if the acceleration equation with Λ=0\Lambda=0Λ=0 and (ρ+ρΛ, p−ρΛ)(\rho+\rho_\Lambda,\ p-\rho_\Lambda)(ρ+ρΛ​, p−ρΛ​) holds at ttt.
  3. The constant density ρΛ\rho_\LambdaρΛ​ with pressure −ρΛ-\rho_\Lambda−ρΛ​ (so wΛ=−1w_\Lambda=-1wΛ​=−1) satisfies the continuity equation at ttt.

This makes precise the remark after Eq. (9): the vacuum stress tensor Tμν(vac)=−Λ(vac)8πGgμνT^{(\rm vac)}_{\mu\nu} = -\frac{\Lambda^{(\rm vac)}}{8\pi G}g_{\mu\nu}Tμν(vac)​=−8πGΛ(vac)​gμν​ coincides with the cosmological-constant term. It also matches the description in §3.7 of Λ\LambdaΛ as a fluid with constant energy density and wΛ=−1w_\Lambda=-1wΛ​=−1.

Formalization Note The equivalence is stated at the level of the background equations (2), (3) and (7), not of the full Einstein tensor equation.

Preamble
import Mathlib
import Definitions.Def_DarkEnergyLCDM_Defs
Formal statement
namespace DarkEnergyLCDM

open Real

theorem vacuum_energy_as_lambda (G K Λ : ℝ) (hG : G ≠ 0) (a ρ p : ℝ → ℝ) (t : ℝ) :
    (FriedmannEq G K Λ a ρ t ↔
      FriedmannEq G K 0 a (fun s => ρ s + Λ / (8 * π * G)) t) ∧
    (AccelerationEq G Λ a ρ p t ↔
      AccelerationEq G 0 a (fun s => ρ s + Λ / (8 * π * G))
        (fun s => p s - Λ / (8 * π * G)) t) ∧
    ContinuityEq a (fun _ => Λ / (8 * π * G)) (fun _ => -(Λ / (8 * π * G))) t := by sorry

end DarkEnergyLCDM
Source
R. von Marttens, J. Alcaniz, S. Carneiro, "A energia escura e os desafios do modelo cosmológico padrão", Cadernos de Astronomia 7(1), 62–76 (2026), https://doi.org/10.47456/Cad.Astro.v7n1.52249, p. 65, Eq. (9) and following text; p. 71, §3.7

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