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.
Stationarity of the adopted total action is equivalent to the Einstein equation with the framework's coupling
Smooth classical domain of the action formulation of the framework: an oriented time-oriented smooth Lorentzian four-manifold, a matter sector whose stress-energy tensor is represented by its action in the Hilbert convention (the supplied scalar-field sector), and compactly supported metric variations. Excludes quantum gravity, boundaries and junction terms, non-smooth or distributional sources, and constraint or propagation claims; no empirical statement and no existence claim for solutions. Every conclusion is a conditional consequence of the adopted action postulate and the mathematics of the framework.
Statement
Adopt the action formulation of the framework, that is, the action density and matter sectors of Adopted classical gravitational action and variational field law, for a model whose geometric data and matter sector satisfy Adopted spacetime model and classical domain of the gravitational framework and Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions; let be oriented with metric volume form and metric-selected connection (Oriented smooth manifolds and oriented charts, The metric volume form, current flux through 3-faces and finite-chain charges, Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), and suppose the model's matter sector supplies a stress-energy tensor field on (Stress-energy tensor field of a model, Smooth covariant 2-tensor fields on a smooth manifold) which is the Hilbert stress-energy tensor of the matter action at with respect to (The Hilbert stress-energy tensor of a metric-dependent action); in particular this holds in the scalar-field sector, where the model is of The scalar-field matter model of the classical gravitational framework and the claim is supplied by First variation, Hilbert tensor and conservation of the scalar-field model clause (b).
(a) Equivalence. With and the Einstein tensor (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors), the following are equivalent:
- the metric is stationary for the total action difference under every smooth family of smooth Lorentzian metrics with and compactly supported variation;
- at every point of .
(b) The two presentations agree. Consequently, in the action presentation
the classical field law of clause (iv) of
Adopted classical gravitational action and variational field law has the same equation form
as the field law adopted in the
direct-equation presentation Adopted Einstein field equation in the direct-equation presentation; the two
presentations are equivalent descriptions of one classical field law, and a
model adopts exactly one of them. In the prescribed- sectors (dust and
perfect fluid) the equation is adopted directly, as recorded in clause (iii)
of Adopted classical gravitational action and variational field law, and its consistency condition
is derived separately in pthm-gr-einstein-consistency-and-energy-conditions
on the owning page gr-einstein-and-matter.
Facts & Assumptions
Given: The adopted action formulation of Adopted classical gravitational action and variational field law for a model with an oriented , matter sector with Hilbert tensor at , and the constants of SI unit and coordinate conventions of the classical gravitational framework.
For every chart-supported smooth family of smooth Lorentzian metrics at with compactly supported variation and every constant , the compactly supported chart action difference satisfies with , and every smooth symmetric compactly supported arises from such a family (First variation of the Einstein-Hilbert density under compactly supported metric variations, and of the timelike length functional clauses (a),(e)).
The matter action's metric variation is represented by : (The Hilbert stress-energy tensor of a metric-dependent action clause (b)). In the scalar sector this is proved in First variation, Hilbert tensor and conservation of the scalar-field model clause (b).
The action differences of clauses (ii)-(iii) of Adopted classical gravitational action and variational field law are integrals of compactly supported smooth top forms. Finite smooth cutoffs with compact chart supports and sum near any compact set exist, and they define the global integral by a finite sum independently of the cutoffs. For a chart-supported top form this global integral agrees with its chart integral; this applies both to the localized gravitational variations and to the Hilbert convention (Finite chart localization gives choice-free integration and compact Stokes, The metric volume form, current flux through 3-faces and finite-chain charges).
If a continuous symmetric covariant -tensor field on a chart domain satisfies for every smooth symmetric compactly supported , then (A continuous symmetric coefficient orthogonal to every compactly supported variation vanishes).
is the sum of the action differences of Adopted classical gravitational action and variational field law clauses (ii)-(iii), and the constants satisfy (SI unit and coordinate conventions of the classical gravitational framework).
Proof
(Einstein-Hilbert part for arbitrary compact support.) Let be an arbitrary family in the Statement, equal to off a compact set , and put , . By [L3] choose finitely many smooth cutoffs with compact chart supports and near . Put , so and with . The derivative at of the top form is linear in and its first and second derivatives: this follows directly from the inverse-metric, connection and Ricci variation formulas of First variation of the Einstein-Hilbert density under compactly supported metric variations, and of the timelike length functional clauses (a)-(d), applied locally: near any point one may multiply by a compactly chart-supported cutoff equal to on a neighborhood of that point. For small parameter values the resulting metric remains Lorentzian by compactness and agrees with the original family on that neighborhood, so the same local variation jets and formulas apply. Thus this derivative for is the sum of its derivatives for the , including all derivatives of the cutoffs; none is discarded. Each is realizable by a Lorentzian family after restricting its parameter interval about , by [L1]. For each such chart-supported family [L1] gives the integrated derivative , where chart and global integrals agree by [L3]. Differentiation of the original global action difference is legitimate by the same finite localization: in each compact chart support its smooth coefficient and parameter derivative are uniformly continuous on a compact parameter interval times that support, so difference quotients converge uniformly to the derivative and hence their integrals converge. Finite linearity and therefore give No single chart containing and no partition on the whole noncompact manifold are required.
(Matter part.) By [L2], .
(Total variation.) Adding steps 1.1 and 1.2 and using by [L5],
(Coefficient vanishes.) Suppose is stationary in the sense of clause (a)(1): the derivative in step 2.1 vanishes for every smooth family with compactly supported variation. Every smooth symmetric test field compactly supported in a chosen chart is realizable by [L1], so for the continuous symmetric field and every smooth symmetric compactly supported ; [L4] gives on every chart, that is, . Conversely, if the equation holds, the integrand of step 2.1 vanishes identically for every family, so the derivative vanishes and is stationary. This proves the equivalence (a).
(Identification of the presentations.) Clause (b) is now immediate: clause (iv) of Adopted classical gravitational action and variational field law states the variational principle whose equation form is, by step 3.1, exactly , the equation adopted in Adopted Einstein field equation in the direct-equation presentation clause (i); the prescribed- sectors adopt that same equation directly by clause (iii) of the action postulate. Since each model adopts exactly one presentation, no model uses both as independent premises.
Remarks
-
Conditional content. The theorem is a deduction from the adopted action postulate and the mathematics of the variational calculus; it does not assert that nature realizes the action principle, that the matter sector is realized physically, or that any solution of the equation exists.
-
No empirical premises. No experiment, measurement or empirical estimate enters this item, and no empirical qualification is inherited by its conclusions.
-
Boundary terms excluded. The equivalence is stated for compactly supported metric variations; the Einstein-Hilbert action of a region with boundary would require additional boundary terms and is not covered here.
Depends on
Adopted classical gravitational action and variational field law
Adopted Einstein field equation in the direct-equation presentation
Adopted spacetime model and classical domain of the gravitational framework
Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions
The scalar-field matter model of the classical gravitational framework
First variation, Hilbert tensor and conservation of the scalar-field model
The Hilbert stress-energy tensor of a metric-dependent action
Uniqueness of the Hilbert stress-energy tensor
First variation of the Einstein-Hilbert density under compactly supported metric variations, and of the timelike length functional
A continuous symmetric coefficient orthogonal to every compactly supported variation vanishes
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Metric compatibility, torsion freedom and the metric-selected connection class
Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
The derivative of the metric density and the chart formula for the divergence of a vector field
The metric volume form, current flux through 3-faces and finite-chain charges
Stress-energy tensor field of a model
Smooth covariant 2-tensor fields on a smooth manifold
SI unit and coordinate conventions of the classical gravitational framework
Finite chart localization gives choice-free integration and compact Stokes
Oriented smooth manifolds and oriented charts
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 4: variation of the total action (4.68)-(4.70) giving Einstein's equations with the energy-momentum tensor (4.70), printed pp. 117-118 (PDF pp. 124-125)
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision), sections 9.2-9.3: the variation (9.23)-(9.25) of the Einstein-Hilbert action, the definition (9.28)-(9.29) of T^{ab} and the resulting equation (9.33)-(9.34), printed pp. 115-117 (PDF pp. 116-118)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 4.5.2: varying the combined action and reading off G_{mu nu}+Lambda g_{mu nu}=8 pi G T_{mu nu} from (4.46)-(4.47), printed pp. 182-183 (PDF pp. 189-190)