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.
Vacuum conformal constraint data
Pure mathematical definition of compact vacuum, zero-cosmological-constant conformal initial data and its algebraic constraint residuals; no embedded development, existence theorem, or empirical claim is asserted.
Definition
Let be a nonempty smooth three-manifold without boundary that is compact: for every family of open subsets of with , there is a finite subset such that . In this item, “vacuum” means that the stress-energy tensor is zero and the cosmological constant is fixed at . Let be a smooth Riemannian metric on , let be a smooth symmetric covariant two-tensor field, let be constant, and let satisfy at every . Use the positive scalar as a dimensionless conformal factor.
Write for the Levi-Civita connection of and for that of the metric defined below. On covariant tensor fields, these symbols also denote their induced product connections, with the dual and tensor-factor rules of the product-connection supplier in Definition references. In a chart, denotes the inverse matrix to . It is smooth because and the matrix inverse is the adjugate divided by the determinant. For any smooth Riemannian metric on , with Levi-Civita connection , define In a chart, denotes the components of . Define and . In particular, , with the same curvature sign convention. Define the scalar Laplacian by where are the Christoffel symbols of , given by the Levi-Civita Christoffel formula in Definition references. The curvature sign is the one displayed above. All traces, norms, raising of indices and contractions in this item use the metric indicated by the subscript. In particular, The tensor is transverse-traceless (TT) with respect to when it is symmetric and both displayed trace and divergence vanish. The input tensor in this definition is required to be TT.
Define Because , is a smooth Riemannian metric; because and are symmetric, is a smooth symmetric tensor. Here is the candidate induced Riemannian metric and is the candidate second fundamental form, with the library convention when the data are induced by a spacelike hypersurface with future unit normal . The pair is vacuum conformal constraint data. It is abstract data on ; no embedding into a spacetime is part of this definition. For its embedded Lorentzian interpretation assume the Axiom of Countable Choice , as in the supplied smooth tangent-bundle convention; the algebraic tensor definitions themselves use no choice principle. Define the -trace, squared norm and divergence by With computed using , define the Hamiltonian and momentum residuals The data satisfy the vacuum constraint equations when and . For an embedded hypersurface, these are the normal and normal-tangential Einstein constraints in the specified convention.
Tensoriality of curvature and basis-independent contraction make these scalar curvatures independent of the chart. For dimensional bookkeeping in the SI length convention, , , and . Thus all terms in the scalar constraint equation have units .
Definition references
Smooth manifolds and their smooth charts
Riemannian metric and riemannian manifold
Product connection on tensor and hom bundles
Fundamental theorem of riemannian geometry
Christoffel symbols of an affine connection
Christoffel formula for the levi civita connection
Curvature of an affine connection
Curvature is a type (1,3) tensor
The contraction of a mixed tensor
Contraction is independent of the basis formula
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
Sums, scalar multiples, products and quotients: , , , and when
Euclidean maps are closed under componentwise algebra and composition
Identity maps and composites of smooth maps are smooth
The Axiom of Countable Choice ()
Spacelike initial data, the constraint equations, developments and maximal developments
Facts & Assumptions
Given: A nonempty compact smooth three-manifold, a smooth Riemannian metric , a smooth symmetric TT covariant tensor , a positive smooth scalar , and a constant . For the embedded Lorentzian constraint interpretation assume .
The Axiom of Countable Choice (), Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model: is the axiom that every countable family of nonempty sets has a choice function; the Lorentzian time-orientation and smooth normal-field conventions use this assumption for the embedded interpretation.
Smooth manifolds and their smooth charts, A smooth tensor field: a smooth manifold has smooth coordinate charts, and a smooth tensor field has smooth coordinate components.
Riemannian metric and riemannian manifold: a Riemannian metric is a smooth symmetric covariant two-tensor that is positive definite at every point.
Fundamental theorem of riemannian geometry: each smooth Riemannian metric has a unique Levi-Civita connection.
Integer powers : negative integer powers are defined for nonzero bases; Laws of integer exponents gives their product and quotient identities.
Sums, scalar multiples, products and quotients: , , , and when , Euclidean maps are closed under componentwise algebra and composition: the quotient rule holds for a nonzero denominator, and finite sums, products and compositions of maps remain for every finite .
Identity maps and composites of smooth maps are smooth: the composition of smooth maps between smooth manifolds is smooth.
Christoffel formula for the levi civita connection: the Christoffel symbols of a smooth Riemannian metric are .
Curvature is a type (1,3) tensor: the curvature defined from an affine connection is a tensor field of type .
The contraction of a mixed tensor: contraction pairs one covariant and one contravariant slot of a tensor.
Contraction is independent of the basis formula: tensor contraction has the same value in every basis.
Spacelike initial data, the constraint equations, developments and maximal developments: the library uses for the second fundamental form, and the vacuum constraints have and vanishing stress-energy.
Gauss-Codazzi decomposition in Gaussian normal coordinates and the constraint equations in terms of the induced metric and second fundamental form: in that convention the normal and normal-tangential Einstein projections give the Hamiltonian and momentum constraint residuals.
Product connection on tensor and hom bundles: for a smooth function , its differential is the covector field defined by . The induced dual connection on covectors gives ; contracting this covariant tensor with is a chart-independent scalar.
Proof
For each integer , induction by the product rule gives , and the quotient rule on gives ; iterating this identity shows that every derivative of is a constant multiple of a negative integer power, hence is continuous on . The map is a polynomial. Thus both maps are smooth there; [F5] gives their regularity at every finite order and [F6] makes their composites with smooth. Hence is smooth, symmetric and positive definite, because for every nonzero , by [F2]. The same rules show that is smooth and symmetric. The Riemannian connection theorem [F3] supplies both and .
In each chart and ; the adjugate entries are polynomials in the smooth metric components [F1], and the reciprocal is smooth by the same quotient-rule induction as in the earlier proof step 1.1 and finite-order algebra closure [F5]. Thus is smooth; is smooth by step 1.1. Formula [F7] therefore makes the Christoffel symbols smooth, so the displayed Laplacian is defined for smooth . By [F13] it is the trace of the covariant derivative of , so its value is independent of the chart. By [F8] curvature is tensorial, and by [F9, F10] its Ricci and scalar contractions do not depend on the chart. The same basis-independent contractions define the traces and squared norms; all derivative terms use the connections supplied by [F3].
For data induced by an embedded spacelike hypersurface, the convention in [F11] fixes the sign of , and [F12] gives precisely the stated Hamiltonian and momentum residuals when and stress-energy vanishes. The abstract data definition itself makes no embedding or development assertion.
Depends on
Smooth manifolds and their smooth charts
A smooth tensor field
Riemannian metric and riemannian manifold
Levi civita connection
Product connection on tensor and hom bundles
Fundamental theorem of riemannian geometry
Christoffel symbols of an affine connection
Christoffel formula for the levi civita connection
Curvature of an affine connection
Curvature is a type (1,3) tensor
The contraction of a mixed tensor
Contraction is independent of the basis formula
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
Integer powers
Laws of integer exponents
Sums, scalar multiples, products and quotients: , , , and when
Euclidean maps are closed under componentwise algebra and composition
Identity maps and composites of smooth maps are smooth
The Axiom of Countable Choice ()
Spacelike initial data, the constraint equations, developments and maximal developments
Gauss-Codazzi decomposition in Gaussian normal coordinates and the constraint equations in terms of the induced metric and second fundamental form
Dependency tree · 2 levels
Sources
- É. Gourgoulhon, 3+1 Formalism and Bases of Numerical Relativity, Lecture Notes in Physics 846 (2012; author preprint arXiv:gr-qc/0703035v1), §6.3.3, §§6.4.1–6.4.2, §§6.5.2–6.5.3, and §§8.2.2–8.2.4
- R. Bartnik and J. Isenberg, The Constraint Equations, in The Einstein Equations and the Large Scale Behavior of Gravitational Fields (Birkhäuser, 2004), arXiv:gr-qc/0405092v1