Alphabeta Math
ExampleConstruction: AI-adaptedVerification: AI-generatedPipeline-generatedprecheck passjudge pass (gpt-6.1-sol)
How statement and proof provenance work

The first chip identifies the source of the statement or construction; the second identifies the source of its local proof or verification.

  • Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
  • AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
  • AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.

These labels describe origin, not correctness: citations and verification chips remain separate evidence.

Null plane-wave scalar field and its conserved stress-energy tensor

Example

Let k≠0 be a null covector, ηabkakb=0, with k♯ future, let f:R→R be smooth, θ0∈R, and let φ(x):=f(kaxa+θ0) in an inertial chart; take V≡0 and K>0. Then φ solves the massless scalar-field equation of First variation of the scalar-field action and the Euler-Lagrange equation, and its Hilbert stress-energy tensor is the conserved tensor Tab=Kf′(kaxa+θ0)2 kakb, a positive multiple of the rank-one tensor k♯⊗k♯, whose generating vector k♯ is nonzero and future null, wherever f′≠0 and the zero tensor wherever f′=0.

Facts & Assumptions

Given: The affine Minkowski model with inertial chart x, constant ηab=ηab=diag⁡(−1,1,1,1) (Oriented time-oriented affine Minkowski space (the spacetime primitives), Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space), coordinate partials ∂a (Directional derivatives and partial derivatives of a map U⊆Rm→Rn); a nonzero null covector k with k♯ future (kaka=0, ka=ηabkb≠0, k0>0) (Timelike, null, spacelike and causal vectors of a Lorentz vector space, Time orientation, future and past timelike/null/causal vectors, and the closed cones); smooth f, θ:=kaxa+θ0; V≡0, K>0; φ=f∘θ, a smooth scalar field (C^k tensor fields on affine Minkowski space and their inertial components).

[F1]

Chain rule: ∂aφ=f′(θ)ka and ∂a∂bφ=f′′(θ)kakb. (The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a), Directional derivatives and partial derivatives of a map U⊆Rm→Rn)

[F2]

Scalar-field equation and Hilbert tensor: the field equation of the model with potential V is □φ=V′(φ), and the Hilbert tensor of the density with this V is Tab=K[∂aφ∂bφ−ηab(12∂dφ∂dφ+V(φ))]. (First variation of the scalar-field action and the Euler-Lagrange equation, The Hilbert stress-energy tensor of the scalar-field action on flat spacetime)

[F3]

Divergence identity: ∂aTab=K(□φ−V′(φ))∂bφ; consequently any solution of the field equation has conserved Hilbert tensor. (Divergence identity for the scalar-field stress-energy tensor)

Verification

technique · direct
1.1F1F2given

The field solves the massless equation. By [F1], ∂aφ=f′(θ)ka and ∂a∂bφ=f′′(θ)kakb; hence □φ=ηab∂a∂bφ=f′′(θ)ηabkakb=0, because k is null. With V≡0 this is exactly the scalar-field equation □φ=V′(φ) of [F2].

2.1F1step 1.1given

The stress-energy tensor. Substituting [F1] into the Hilbert formula of [F2] with V≡0 gives ∂aφ∂bφ=f′(θ)2kakb and ∂dφ∂dφ=f′(θ)2kdkd=0, hence Tab=Kf′(θ)2kakb, which is symmetric. Wherever f′(θ)≠0 the coefficient Kf′(θ)2 is positive and T is a positive multiple of the rank-one tensor k♯⊗k♯ with nonzero future null generating vector k♯; wherever f′(θ)=0 all components vanish. For every future unit n, Tabnanb=Kf′(θ)2(kana)2≥0; in the inertial frame, T00=Kf′(θ)2(k0)2≥0 with k0>0.

2.2F3step 1.1

Conservation. Since φ solves the field equation by step 1.1, [F3] gives ∂aTab=0: the plane-wave tensor is conserved on the whole chart domain.

3.1step 2.1step 2.2∎

The example is an explicit conditional computation for the massless scalar model with a null plane-wave profile; it asserts no wave observation, no energy condition beyond the displayed nonnegativity and no measurement.

Depends on

Dependency tree · 2 levels

Sources