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Prop. 2.2: Trautman recovery

Proved
NewtonCartan.recovery

by Alien60 · Oct 20, 2026 · Mathlib 0df444a (Lean v4.33.1)

category-theoryclassical-spacetimegeometrized-newtonian-gravitationnewton-cartanphilosophy-of-physicstheoretical-equivalence

Spacetime is R4\mathbb R^4R4 in a global chart (index 0 = time) with ta=dx0t_a=dx^0ta​=dx0, hab=diag(0,1,1,1)h^{ab}=\mathrm{diag}(0,1,1,1)hab=diag(0,1,1,1); a derivative operator is a smooth symmetric Christoffel field Γabc\Gamma^a{}_{bc}Γabc​; curvature in Malament's convention ξbRabcd=−2∇[c∇d]ξa\xi^bR^a{}_{bcd}=-2\nabla_{[c}\nabla_{d]}\xi^aξbRabcd​=−2∇[c​∇d]​ξa, Rbc=RnbcnR_{bc}=R^n{}_{bcn}Rbc​=Rnbcn​; Γ~=Γ+tbtc∇aφ\tilde\Gamma=\Gamma+t_bt_c\nabla^a\varphiΓ~=Γ+tb​tc​∇aφ is the geometrization; timelike curves have unit tangent taξa=1t_a\xi^a=1ta​ξa=1. If ∇~\tilde\nabla∇~ is a classical spacetime satisfying (1)-(3) for some smooth ρ\rhoρ, there are a smooth φ\varphiφ and a flat compatible ∇\nabla∇ such that the timelike geodesics of ∇~\tilde\nabla∇~ are exactly the curves with ξn∇nξa=−∇aφ\xi^n\nabla_n\xi^a=-\nabla^a\varphiξn∇n​ξa=−∇aφ, and ∇a∇aφ=4πρ\nabla^a\nabla_a\varphi=4\pi\rho∇a∇a​φ=4πρ.

Preamble
import Definitions.Def_NewtonCartan_defs

open scoped ContDiff
Formal statement
namespace NewtonCartan

/-- **Prop. 2.2 (Trautman).** Let `(ℝ⁴, t_a, h^{ab}, ∇̃)` be a classical spacetime satisfying
conditions (1)–(3) of Prop. 2.1 for some smooth `ρ`. Then there are a smooth `φ` and a flat derivative
operator `∇` such that `(ℝ⁴, t_a, h^{ab}, ∇)` is a classical spacetime, the timelike geodesics of `∇̃`
are exactly the curves with `ξ^n ∇_n ξ^a = -∇^a φ`, and `∇, φ` satisfy Poisson's equation. -/
theorem recovery (Γt : Conn) (ρ : E → ℝ) (hΓt : IsClassical Γt) (hρ : ContDiff ℝ ∞ ρ)
    (hcurv : CurvConds Γt ρ) :
    ∃ (Γ : Conn) (φ : E → ℝ), IsNG Γ φ ∧ SameTrajectories Γ φ Γt ∧ Poisson Γ φ ρ := by sorry

end NewtonCartan
Source
J. O. Weatherall, Are Newtonian Gravitation and Geometrized Newtonian Gravitation Theoretically Equivalent?, Erkenntnis 81 (2016) 1073-1091, https://arxiv.org/abs/1411.5757, Prop. 2.2 (pp. 4-5); D. B. Malament, Topics in the Foundations of General Relativity and Newtonian Gravitation Theory (2012), Ch. 4, Prop. 4.2.5
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What the Lean code literally says, in plain math · claude-opus-5-5

For every classical Γt\Gamma_tΓt​ and every C∞C^\inftyC∞ ρ\rhoρ with CurvConds(Γt,ρ\Gamma_t,\rhoΓt​,ρ), there exist a connection Γ\GammaΓ and function ϕ\phiϕ with Γ\GammaΓ classical and flat, ϕ∈C∞\phi\in C^\inftyϕ∈C∞, SameTrajectories(Γ,ϕ,Γt\Gamma,\phi,\Gamma_tΓ,ϕ,Γt​), and ∑hab∇a∇bϕ=4πρ\sum h^{ab}\nabla_a\nabla_b\phi=4\pi\rho∑hab∇a​∇b​ϕ=4πρ everywhere.

Flags: hypotheses satisfiable (Γt=0,ρ=0\Gamma_t=0,\rho=0Γt​=0,ρ=0). ρ\rhoρ-smoothness is redundant (follows from (1)). The true statement needs contractibility of R4\mathbb R^4R4 (Trautman/Malament 4.2.x); a genuinely hard existence theorem, no hypotheses appear missing. No uniqueness asserted.

Human review
  • Endorsed by Shuze Chen · Oct 21, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Alien60 · Oct 21, 2026

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

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