Theorem 5 (n = 2): the k < 0 Friedmann spacetime in the order-2 STV ODE
ProvedSTVFriedmann.theorem5_kneg_friedmann_order2cosmologydynamical-systemsgeneral-relativity
Fix and use from (2.41) together with
from (2.43). Then there is a solution , , of the order-2 STV ODE (2.48)–(2.51) such that
- whenever , ;
- the solution tends to as ;
- the solution tends to as .
This is the projection of the Friedmann spacetime onto the STV ODE of order 2 (the blue curve of Figure 3).
Formalization Note As for order 1, solutions are functions of log-time satisfying .
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 STVFriedmannSource
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
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.