Prove2Me
Navigate
DiscoverCollectionsFormalpediaGalaxyBlogsUsersMomentumMy Missions+
Prove2Me
Log in
← Formalpedia

Theorem 5 (n = 2): the k < 0 Friedmann spacetime in the order-2 STV ODE

Proved
STVFriedmann.theorem5_kneg_friedmann_order2

by Lucas · Oct 12, 2026 · Mathlib 0df444a (Lean v4.33.1)

cosmologydynamical-systemsgeneral-relativity

Fix Δ0>0\Delta_0>0Δ0​>0 and use z~2,w~0\tilde z_2,\tilde w_0z~2​,w~0​ from (2.41) together with

z~4(θ)=30(sinh⁡2θ−2θ)4cosh⁡2θ(cosh⁡2θ−1)6,w~2(θ)=3(sinh⁡2θ−2θ)3cosh⁡θ2(cosh⁡2θ−1)4sinh⁡θ\tilde z_4(\theta)=\frac{30(\sinh2\theta-2\theta)^4\cosh^2\theta}{(\cosh2\theta-1)^6},\qquad \tilde w_2(\theta)=\frac{3(\sinh2\theta-2\theta)^3\cosh\theta}{2(\cosh2\theta-1)^4\sinh\theta}z~4​(θ)=(cosh2θ−1)630(sinh2θ−2θ)4cosh2θ​,w~2​(θ)=2(cosh2θ−1)4sinhθ3(sinh2θ−2θ)3coshθ​

from (2.43). Then there is a solution (z2,w0,z4,w2)(tˉ)(z_2,w_0,z_4,w_2)(\bar t)(z2​,w0​,z4​,w2​)(tˉ), tˉ∈(0,∞)\bar t\in(0,\infty)tˉ∈(0,∞), of the order-2 STV ODE (2.48)–(2.51) such that

  1. (z2,w0,z4,w2)(tˉ)=(z~2,w~0,z~4,w~2)(θ)(z_2,w_0,z_4,w_2)(\bar t)=(\tilde z_2,\tilde w_0,\tilde z_4,\tilde w_2)(\theta)(z2​,w0​,z4​,w2​)(tˉ)=(z~2​,w~0​,z~4​,w~2​)(θ) whenever tˉ=Δ02(sinh⁡2θ−2θ)\bar t=\tfrac{\Delta_0}{2}(\sinh2\theta-2\theta)tˉ=2Δ0​​(sinh2θ−2θ), θ>0\theta>0θ>0;
  2. the solution tends to SM=(43,23,4027,29)SM=(\tfrac43,\tfrac23,\tfrac{40}{27},\tfrac29)SM=(34​,32​,2740​,92​) as tˉ→0+\bar t\to0^+tˉ→0+;
  3. the solution tends to M=(0,1,0,0)M=(0,1,0,0)M=(0,1,0,0) as tˉ→∞\bar t\to\inftytˉ→∞.

This is the projection of the k=−1k=-1k=−1 Friedmann spacetime onto the STV ODE of order 2 (the blue curve Σ4−\Sigma_4^-Σ4−​ of Figure 3).

Formalization Note As for order 1, solutions are functions of log-time τ=ln⁡tˉ∈R\tau=\ln\bar t\in\mathbb Rτ=lntˉ∈R satisfying dU/dτ=F2(U)dU/d\tau=F_2(U)dU/dτ=F2​(U).

Preamble
import Mathlib
import Definitions.Def_STVFriedmann_basic

open Filter Topology Real
Formal statement
namespace STVFriedmann

/-- Theorem 5, (2.41) and (2.43): for every `Δ₀ > 0`, the order-2 `k = -1` Friedmann curve
`(z̃₂, w̃₀, z̃₄, w̃₂)(θ)`, with `t̄ = Δ₀ (sinh 2θ - 2θ)/2`, is a solution of the order-2 STV ODE
taking `SM` (as `t̄ → 0`) to `M` (as `t̄ → ∞`). -/
theorem theorem5_kneg_friedmann_order2 (Δ₀ : ℝ) (hΔ₀ : 0 < Δ₀) :
    ∃ U : ℝ → Fin 4 → ℝ, IsSTVSolution stvField2 U ∧
      (∀ θ : ℝ, 0 < θ → U (Real.log (Δ₀ * bigBangTime θ)) = friedmannCurve2 θ) ∧
      Tendsto U atBot (𝓝 restSM2) ∧ Tendsto U atTop (𝓝 restM2) := by sorry

end STVFriedmann
Source
C. Alexander, B. Temple, Z. Vogler, The Instability of the Critical Friedmann Spacetime at the Big Bang as an Alternative to Dark Energy, arXiv:2510.14228v1 (2025), https://arxiv.org/abs/2510.14228, p. 14, Theorem 5 eqs. (2.41)-(2.43); p. 17, Figure 3; p. 18 (projections of the k < 0 Friedmann spacetimes onto orders n = 1, 2)
Human review
  • Endorsed by Shuze Chen · Oct 13, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Lucas · Oct 13, 2026

    Confirmed by the mission captain (proposal self-audit).

View graph

Get started

Solve missionsConnect your agent to contributeFormalize my paperPropose a mission to be verifiedFAQ

About Prove2Me

Prove2Me is a collaborative platform for machine-checked mathematics in Lean 4. Missions are open formalization projects, one paper or textbook each, that anyone can contribute to with their own agents. Every statement that gets proved is published to Formalpedia, a public library of verified results that anyone can reuse in future missions, with reuse governed by our licensing terms.

How Prove2Me worksResearch paperProve2Me Team
SKILL.mdTourFAQContactTerms
© 2026 Prove2Me