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Identity (12a): the gravitational energy-momentum identity

Proved
EinsteinGrossmann1913.gravitational_energy_momentum_identity

by Lucas · Oct 9, 2026 · Mathlib 0df444a (Lean v4.33.1)

entwurf-theorygeneral-relativityhistory-of-physicstensor-calculus

Let gμνg_{\mu\nu}gμν​ be a fundamental tensor on R4\mathbb R^4R4 (twice continuously differentiable, symmetric, with g=det⁡(gμν)<0g=\det(g_{\mu\nu})<0g=det(gμν​)<0), let γμν\gamma_{\mu\nu}γμν​ be its reciprocal, and let κ≠0\kappa\neq0κ=0. With ϑμν\vartheta_{\mu\nu}ϑμν​ the stress-energy tensor of the gravitational field (eq. (13)) and Δμν(γ)\Delta_{\mu\nu}(\gamma)Δμν​(γ) the operator of eq. (15), for every σ=1,2,3,4\sigma=1,2,3,4σ=1,2,3,4 and every point,

∑μν∂∂xν{−g gσμ κϑμν}=12∑μν−g ∂gμν∂xσ{−Δμν(γ)+κϑμν}.\sum_{\mu\nu}\frac{\partial}{\partial x_\nu}\Big\{\sqrt{-g}\,g_{\sigma\mu}\,\kappa\vartheta_{\mu\nu}\Big\}=\tfrac12\sum_{\mu\nu}\sqrt{-g}\,\frac{\partial g_{\mu\nu}}{\partial x_\sigma}\Big\{-\Delta_{\mu\nu}(\gamma)+\kappa\vartheta_{\mu\nu}\Big\}.μν∑​∂xν​∂​{−g​gσμ​κϑμν​}=21​μν∑​−g​∂xσ​∂gμν​​{−Δμν​(γ)+κϑμν​}.

This is the identity (12) of the paper rewritten with the abbreviations (13) and (15). It is a pure differential identity in gμνg_{\mu\nu}gμν​, valid for every metric field, and it is the step from which the field equations (18) and the conservation law (19) are read off.

Formalization Note κϑμν\kappa\vartheta_{\mu\nu}κϑμν​ does not depend on κ\kappaκ; κ≠0\kappa\neq0κ=0 is assumed because ϑμν\vartheta_{\mu\nu}ϑμν​ is defined with the factor 1/(2κ)1/(2\kappa)1/(2κ).

Preamble
import Mathlib
import Definitions.Def_EinsteinGrossmann1913_Defs
Formal statement
namespace EinsteinGrossmann1913

theorem gravitational_energy_momentum_identity (κ : ℝ) (hκ : κ ≠ 0) (g : Field2)
    (hg : IsMetricField g) (σ : Fin 4) (x : Coord) :
    ∑ μ : Fin 4, ∑ ν : Fin 4,
        pd ν (fun y => sqrtNegDet g y * g y σ μ * (κ * gravStressEnergy κ g y μ ν)) x
      = (1 / 2) * ∑ μ : Fin 4, ∑ ν : Fin 4,
          sqrtNegDet g x * pd σ (fun y => g y μ ν) x
            * (-entwurfDelta g x μ ν + κ * gravStressEnergy κ g x μ ν) := by sorry

end EinsteinGrossmann1913
Source
A. Einstein and M. Grossmann, "Entwurf einer verallgemeinerten Relativitätstheorie und einer Theorie der Gravitation", B. G. Teubner, Leipzig und Berlin 1913 (Separatabdruck aus Zeitschrift für Mathematik und Physik 62), Part I (Physikalischer Teil, A. Einstein), §5, pp. 15–16, eqs. (12), (13), (15) and (12a).
Read-back

What the Lean code literally says, in plain math · Aristotle (Harmonic) - same agent as the drafter; non-blind

Non-blind read-back — not independent testimony. This read-back was written by the same agent (Aristotle, by Harmonic) that drafted the Lean statements it describes, with full knowledge of the source paper and of the intended meaning. It is not the output of a blind, independent auditor, and no reviewer should treat it as such. Compare it against the Lean code yourself.

Let κ\kappaκ be a real number with κ≠0\kappa\neq0κ=0. ggg is an arbitrary map assigning to every point x∈R4x\in\mathbb R^4x∈R4 a real 4×44\times44×4 matrix (gμν(x))(g_{\mu\nu}(x))(gμν​(x)), and the hypothesis IsMetricField ggg requires exactly: every entry x↦gμν(x)x\mapsto g_{\mu\nu}(x)x↦gμν​(x) is C2C^2C2 on all of R4\mathbb R^4R4; gμν(x)=gνμ(x)g_{\mu\nu}(x)=g_{\nu\mu}(x)gμν​(x)=gνμ​(x) for all x,μ,νx,\mu,\nux,μ,ν; and det⁡(gμν(x))<0\det(g_{\mu\nu}(x))<0det(gμν​(x))<0 for every xxx. No signature condition beyond the sign of the determinant is imposed. Fix an index σ\sigmaσ and a point x∈R4x\in\mathbb R^4x∈R4. Throughout, ∂if(x)\partial_i f(x)∂i​f(x) is the Fréchet derivative of fff at xxx applied to the iii-th standard basis vector (by convention it is 000 wherever fff is not differentiable), γμν(x)\gamma_{\mu\nu}(x)γμν​(x) denotes the entries of the matrix inverse of (gμν(x))(g_{\mu\nu}(x))(gμν​(x)), −g\sqrt{-g}−g​ is the real square root of −det⁡(gμν(x))-\det(g_{\mu\nu}(x))−det(gμν​(x)), and 1/01/01/0 is read as 000. Indices range over four values (in the code 0,1,2,30,1,2,30,1,2,3; index 333 plays the role of the source's x4x_4x4​). The statement asserts

∑μ,ν∂ν(y↦−g(y) gσμ(y) κ ϑμν(y))(x)=12∑μ,ν−g(x) ∂σgμν(x) (−Δμν(x)+κ ϑμν(x)),\sum_{\mu,\nu}\partial_\nu\Big(y\mapsto\sqrt{-g}(y)\,g_{\sigma\mu}(y)\,\kappa\,\vartheta_{\mu\nu}(y)\Big)(x)=\frac12\sum_{\mu,\nu}\sqrt{-g}(x)\,\partial_\sigma g_{\mu\nu}(x)\,\Big(-\Delta_{\mu\nu}(x)+\kappa\,\vartheta_{\mu\nu}(x)\Big),μ,ν∑​∂ν​(y↦−g​(y)gσμ​(y)κϑμν​(y))(x)=21​μ,ν∑​−g​(x)∂σ​gμν​(x)(−Δμν​(x)+κϑμν​(x)),

where

ϑμν=−12κ∑α,β,τ,ρ(γαμγβν ∂αgτρ ∂βγτρ−12γμνγαβ ∂αgτρ ∂βγτρ)\vartheta_{\mu\nu}=-\frac{1}{2\kappa}\sum_{\alpha,\beta,\tau,\rho}\Big(\gamma_{\alpha\mu}\gamma_{\beta\nu}\,\partial_\alpha g_{\tau\rho}\,\partial_\beta\gamma_{\tau\rho}-\tfrac12\gamma_{\mu\nu}\gamma_{\alpha\beta}\,\partial_\alpha g_{\tau\rho}\,\partial_\beta\gamma_{\tau\rho}\Big)ϑμν​=−2κ1​α,β,τ,ρ∑​(γαμ​γβν​∂α​gτρ​∂β​γτρ​−21​γμν​γαβ​∂α​gτρ​∂β​γτρ​)

and

Δμν=∑α,β1−g ∂α(γαβ−g ∂βγμν)−∑α,β,τ,ργαβgτρ ∂αγμτ ∂βγνρ.\Delta_{\mu\nu}=\sum_{\alpha,\beta}\frac{1}{\sqrt{-g}}\,\partial_\alpha\big(\gamma_{\alpha\beta}\sqrt{-g}\,\partial_\beta\gamma_{\mu\nu}\big)-\sum_{\alpha,\beta,\tau,\rho}\gamma_{\alpha\beta}g_{\tau\rho}\,\partial_\alpha\gamma_{\mu\tau}\,\partial_\beta\gamma_{\nu\rho}.Δμν​=α,β∑​−g​1​∂α​(γαβ​−g​∂β​γμν​)−α,β,τ,ρ∑​γαβ​gτρ​∂α​γμτ​∂β​γνρ​.

The identity is asserted for every such ggg, every σ\sigmaσ and every xxx; no matter tensor or field equation is involved.

Human review
  • Endorsed by Shuze Chen · Oct 10, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Lucas · Oct 10, 2026

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

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