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Local existence for the reduced Einstein equation from Cauchy data on a spacelike slice
Statement
Assume Countable Choice (The Axiom of Countable Choice ()), carrying the hypotheses of the analytic suppliers used below.
Let be a smooth four-manifold carrying a chart whose domain contains the slice , let be a smooth background metric on with its Levi--Civita connection , and let be a smooth symmetric covariant -tensor on together with the background-covariant derivatives needed below (the matter field data). Suppose smooth functions on are given such that:
- is a smooth field of Lorentzian bilinear forms on the restricted spacetime tangent bundle , whose restriction to is positive definite. Write for its components in the given spacetime chart; its inverse components satisfy and the spatial block is positive definite;
- is symmetric and agrees on with the components of for some smooth extension of to ;
- the harmonic-gauge condition holds on for the pair (The harmonic gauge vector, the reduced Einstein equation and the Einstein residual).
Then there is an open neighborhood of and a smooth metric on with and , solving the reduced Einstein equation with the given background and matter tensor (The harmonic gauge vector, the reduced Einstein equation and the Einstein residual) on .
Facts & Assumptions
Given: Countable Choice and the chart and slice, the background metric , the matter tensor , and data satisfying conditions 1--3.
The reduced Einstein equation is equivalent, on a region where the metric is Lorentzian, and is positive definite, to a first-order quasilinear system for whose coefficient of the time derivative is the positive definite block matrix and whose spatial coefficients are symmetric (Principal part of the reduced Einstein operator and its first-order symmetric hyperbolic reduction clause (b)).
Local well-posedness and finite-speed independence for symmetric hyperbolic systems: solutions exist on a neighborhood of the initial slice and are independent, on the domain of dependence, of the way the data and coefficients are extended beyond a coordinate patch (Local well-posedness and finite-speed independence of the extension for symmetric hyperbolic systems on a coordinate neighbourhood, Local existence of Sobolev and classical solutions of a periodic symmetric hyperbolic system, uniform on bounded H^s data); smooth data give smooth solutions (Smooth data give smooth solutions of a periodic symmetric hyperbolic system on the existence interval).
The data are smooth on the slice, and the metric properties and positive definite spatial block persist in a neighborhood of the slice by continuity; a smooth extension of the data to exists ( and smooth maps between smooth manifolds, Smooth covariant 2-tensor fields on a smooth manifold).
Proof
(Reduction to a first-order symmetric hyperbolic initial value problem.) Extend to smooth fields on with at [L3], and set , initially. By [L1] the reduced equation, together with the definition of , is the first-order quasilinear system on ; at the time matrix of is positive definite because and , and positivity persists in an open neighborhood of the slice by [L3].
(Local solution and independence.) Choose a coordinate ball meeting and cut off the data and the coefficient functions outside ; the resulting system is a periodic symmetric hyperbolic system after identifying a neighborhood of with an open subset of and extending by constants. By [L2] it has a smooth solution on a time interval around ; by the finite-speed independence clause of [L2], restricted to the domain of dependence of the solution depends only on the data and coefficients inside the patch, so the local solutions on overlapping balls agree and patch to a solution of on a neighborhood of .
(Return to the second-order equation.) The metric equation gives . Define the spatial derivative residual , initially zero. The transport equation for contains precisely the commutator . Subtracting the background derivative identity for cancels that term and gives a homogeneous linear ODE along each coordinate time line for (in component form ; the derivative-slot connection terms cancel by background torsion-freeness). Its zero initial value forces , as follows by differentiating its Euclidean squared norm, bounding its derivative by a continuous multiple of itself on each compact time segment, and multiplying by the corresponding exponential integrating factor. Thus and throughout the local time collars. Substitution in the metric wave equation recovers the exact reduced Einstein equation with the stated data. This gives the asserted smooth solution.
Remarks
- Role. This is E1's existence theorem for the gauge-reduced equation; E2 supplies the geometric data from and removes the background dependence by geometric uniqueness, and E3 verifies the matter reductions.
Depends on
The Axiom of Countable Choice ()
The harmonic gauge vector, the reduced Einstein equation and the Einstein residual
Principal part of the reduced Einstein operator and its first-order symmetric hyperbolic reduction
Local well-posedness and finite-speed independence of the extension for symmetric hyperbolic systems on a coordinate neighbourhood
Local existence of Sobolev and classical solutions of a periodic symmetric hyperbolic system, uniform on bounded H^s data
Smooth data give smooth solutions of a periodic symmetric hyperbolic system on the existence interval
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons
Smooth covariant 2-tensor fields on a smooth manifold
and smooth maps between smooth manifolds
maps and multi-index derivative notation in Euclidean space
Dependency tree · 2 levels
Sources
- H. Friedrich and A. D. Rendall, The Cauchy Problem for the Einstein Equations, Living Reviews in Relativity 3 (2000), article 1 (arXiv:gr-qc/0002074), Section 5.1 (Local Existence Theorems for the Einstein Equations): harmonic-map gauge, the reduced initial data constructed from (h,chi), the propagation of the gauge by the homogeneous wave system for the gauge residual Delta^alpha, and the local existence theorem
- H. Friedrich and A. D. Rendall, The Cauchy Problem for the Einstein Equations, Living Reviews in Relativity 3 (2000), article 1 (arXiv:gr-qc/0002074), Section 3.1 (Symmetric Hyperbolic Systems): the definition of a quasilinear symmetric hyperbolic system, the finite-dimensional mollifier approximation (3.1) solved by ODE theory, the energy and Moser product/composition estimates, the higher-order energy inequality, uniqueness, the Rellich/Ascoli compactness step and the passage to a classical solution, with Remarks 1-6 on smooth persistence, the continuation criterion, Cauchy stability and the non-identity time matrix