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Vacuum energy density and pressure

Proved
EinsteinFieldEquationsD.vacuumStressEnergy_eq_perfectFluid

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

differential-geometryeinstein-field-equationsgeneral-relativity

The vacuum stress–energy tensor Tμν(vac)=−ΛκgμνT^{(\mathrm{vac})}_{\mu\nu}=-\frac\Lambda\kappa g_{\mu\nu}Tμν(vac)​=−κΛ​gμν​ is the stress–energy tensor of a perfect fluid with constant energy density and isotropic pressure

ρvac=−pvac=Λκ,\rho_{\mathrm{vac}}=-p_{\mathrm{vac}}=\frac\Lambda\kappa,ρvac​=−pvac​=κΛ​,

for any velocity field uuu: Tμν(vac)=(ρvac+pvac)uμuν+pvacgμνT^{(\mathrm{vac})}_{\mu\nu}=(\rho_{\mathrm{vac}}+p_{\mathrm{vac}})u_\mu u_\nu+p_{\mathrm{vac}}g_{\mu\nu}Tμν(vac)​=(ρvac​+pvac​)uμ​uν​+pvac​gμν​.

Preamble
import Mathlib
import Definitions.Def_EinsteinFieldEquationsD_Defs
Formal statement
namespace EinsteinFieldEquationsD

theorem vacuumStressEnergy_eq_perfectFluid {D : ℕ} (g : Tensor2 D) (Λ κ : ℝ) (u : Coord D → Fin D → ℝ) :
    vacuumStressEnergy g Λ κ = perfectFluid g (Λ / κ) (-(Λ / κ)) u := by sorry

end EinsteinFieldEquationsD
Source
Wikipedia, "Einstein field equations", revision oldid=1374672993, https://en.wikipedia.org/w/index.php?title=Einstein_field_equations&oldid=1374672993; section 'Cosmological constant'
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 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.

Here DDD is arbitrary, ggg is an arbitrary matrix-valued function on RD\mathbb{R}^DRD (no assumptions), Λ,κ\Lambda,\kappaΛ,κ are arbitrary reals (including κ=0\kappa=0κ=0, where Λ/κ\Lambda/\kappaΛ/κ is 000), and uuu is an arbitrary field assigning to each point a vector (ua(x))∈RD(u_a(x))\in\mathbb{R}^D(ua​(x))∈RD (no normalization such as gabuaub=−1g^{ab}u_au_b=-1gabua​ub​=−1 is imposed).

Claim. As functions of (x,a,b)(x,a,b)(x,a,b),

−Λκ gab(x)=(Λκ+(−Λκ))ua(x)ub(x)+(−Λκ)gab(x).-\frac\Lambda\kappa\,g_{ab}(x)=\Big(\frac\Lambda\kappa+\Big(-\frac\Lambda\kappa\Big)\Big)u_a(x)u_b(x)+\Big(-\frac\Lambda\kappa\Big)g_{ab}(x).−κΛ​gab​(x)=(κΛ​+(−κΛ​))ua​(x)ub​(x)+(−κΛ​)gab​(x).
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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