Vacuum energy , is equivalent to
ProvedDarkEnergyLCDM.vacuum_energy_as_lambdacosmologymathematical-physics
Let , let be constants, and set . For any functions and any instant :
- The Friedmann equation with constant and density holds at if and only if the Friedmann equation with and density holds at .
- The acceleration equation with and holds at if and only if the acceleration equation with and holds at .
- The constant density with pressure (so ) satisfies the continuity equation at .
This makes precise the remark after Eq. (9): the vacuum stress tensor coincides with the cosmological-constant term. It also matches the description in §3.7 of as a fluid with constant energy density and .
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