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The normal and normal-tangential projections of the field equation are the constraint equations
Statement
Let be a time-oriented smooth Lorentzian four-manifold with metric-selected connection (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), let be a smooth symmetric covariant -tensor field on (Smooth covariant 2-tensor fields on a smooth manifold), let and let be the Einstein tensor of the metric-selected connection (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors). Suppose that the field equation holds at every point of . Let be a spacelike embedded hypersurface with future unit normal field , induced metric and second fundamental form , and let and for , , be the matter data of Spacelike initial data, the constraint equations, developments and maximal developments clause (b). Then:
(a) The tuple satisfies the constraint equations for in the sense of Spacelike initial data, the constraint equations, developments and maximal developments clause (b), equivalently on .
(b) The fields and are smooth on : in every slice chart their expressions in the slice coordinates are .
Facts & Assumptions
Given: A time-oriented smooth Lorentzian four-manifold with metric-selected connection, a smooth symmetric field , constants , a spacelike embedded hypersurface with data of the definition, and a smooth vector field tangent to at the point under consideration.
The Einstein tensor is , a smooth covariant -tensor field on (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors).
The future unit normal of is smooth along and satisfies with ; the induced metric and the second fundamental form of Spacelike initial data, the constraint equations, developments and maximal developments clause (a) are as constructed there (The future unit normal, induced metric and second fundamental form of a spacelike hypersurface clauses (a)-(c), Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (a)).
A covariant -tensor field is a family of bilinear maps varying smoothly in charts; evaluating it on smooth vector fields (or on one smooth field twice) therefore gives a smooth function, and is symmetric (Smooth covariant 2-tensor fields on a smooth manifold, Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).
For every the equation holds at ; both sides are evaluated on pairs of vectors of , so equality is preserved under evaluation on any pair (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, given).
In a slice chart with , the restriction of to is expressible in the slice coordinates with coefficients, because the local extension of [L2] has components in and is evaluated at (Embedded submanifolds and slice charts).
Proof
(Normal projection.) Let and evaluate the field equation at on the pair , an evaluation of the smooth covariant -tensor field of [L1]; by [L4] and [L3], . By [L2], , and by the definition of ; hence .
(Normal-tangential projection.) Let and , and evaluate the field equation at on the pair ; by [L4] and [L3], . By [L2], is tangent to and is normal, so ; hence by the definition of .
(Conclusion for the constraints.) Steps 1.1 and 1.2 give the two displays of clause (a) for arbitrary and , which is exactly the condition defining that satisfies the constraint equations in Spacelike initial data, the constraint equations, developments and maximal developments clause (b).
(Smoothness of the matter data.) In a slice chart as in [L5], the components of the normal, the components of the metric and the components of the stress-energy field are functions of on ; hence and the corresponding contraction of with and have coordinate expressions in the slice coordinates, for every smooth tangent vector field on . Since the slice charts cover , is a smooth function on and a smooth field on (a covariant -tensor field in the sense of the restriction to of the formulas above). This is (b) and completes the proof.
Remarks
- What is and is not claimed. The lemma is a two-line evaluation identity: it says that a solution of the field equation on the ambient manifold has data satisfying the constraint equations. It does not prove that arbitrary data satisfying the constraints admit a development, and it does not derive the equivalent form of the constraints in terms of the induced scalar curvature and the divergence of ; that form requires the Gauss-Codazzi relations and is deferred with the PDE treatment.
- Smoothness. Clause (b) records that the matter data are genuine smooth fields on , which is what the definition asserts; the proof reads the components in slice charts and uses smoothness of from the normal lemma.
Depends on
Spacelike initial data, the constraint equations, developments and maximal developments
The future unit normal, induced metric and second fundamental form of a spacelike hypersurface
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Smooth covariant 2-tensor fields on a smooth manifold
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
Embedded submanifolds and slice charts
Dependency tree · 2 levels
Sources
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision): the Hamiltonian and momentum constraints obtained by projecting the Einstein equation on the normal and tangential directions of the initial surface, section 10.4 printed p. 123 (PDF p. 124)
- E. Gourgoulhon, 3+1 Formalism and Bases of Numerical Relativity, arXiv:gr-qc/0703035 (2007): projection of the Einstein equation with respect to the normal and the hypersurface, sections 4.1-4.2 printed pp. 51-59; the Hamiltonian and momentum constraint equations, section 4.4.3 printed p. 64
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997): the initial value formulation and the constraint equations, printed pp. 122-124 (PDF pp. 129-131)