Quintessence:
ProvedDarkEnergyLCDM.quintessence_hubble_derivativecosmologymathematical-physics
Let be an open interval, a constant, a function with on , a function on , a differentiable potential, and a matter density differentiable on with pressure . Suppose that on :
- (Eq. 13);
- (Klein–Gordon, Eq. 15);
- .
Then at every with ,
This is the second Einstein equation (14) of the quintessence model.
Formalization Note The source prints . That is inconsistent with (13) and (15) by a factor of , and the consistent coefficient is used here. Instants with are excluded because (14) is not a consequence of (13) and (15) there.
Preamble
import Mathlib import Definitions.Def_DarkEnergyLCDM_Defs
Formal statement
namespace DarkEnergyLCDM
open Real
theorem quintessence_hubble_derivative (G : ℝ) (I : Set ℝ) (hI : IsOpen I)
(a ϕ V ρ p : ℝ → ℝ) (ha : ContDiffOn ℝ 2 a I) (ha_pos : ∀ t ∈ I, 0 < a t)
(hϕ : ContDiffOn ℝ 2 ϕ I) (hV : Differentiable ℝ V) (hρ : DifferentiableOn ℝ ρ I)
(hfried : ∀ t ∈ I,
hubble a t ^ 2 = 8 * π * G / 3 * (deriv ϕ t ^ 2 / 2 + V (ϕ t) + ρ t))
(hKG : ∀ t ∈ I, deriv (deriv ϕ) t + 3 * hubble a t * deriv ϕ t + deriv V (ϕ t) = 0)
(hcont : ∀ t ∈ I, ContinuityEq a ρ p t) :
∀ t ∈ I, hubble a t ≠ 0 →
deriv (hubble a) t = -(4 * π * G) * (deriv ϕ t ^ 2 + ρ t + p 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. 71, Eqs. (13)–(15)