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Local existence for the reduced Einstein equation from Cauchy data on a spacelike slice

Statement

Assume Countable Choice ACω (The Axiom of Countable Choice (ACω)), carrying the hypotheses of the analytic suppliers used below.

Let M be a smooth four-manifold carrying a chart (x0=t,x1,x2,x3) whose domain U contains the slice Σ:={t=0}, let gˉ be a smooth background metric on U with its Levi--Civita connection ∇ˉ, and let T be a smooth symmetric covariant 2-tensor on U together with the background-covariant derivatives needed below (the matter field data). Suppose smooth functions gab0,gab1 on Σ∩U are given such that:

  1. g0 is a smooth field of Lorentzian bilinear forms on the restricted spacetime tangent bundle TM∣Σ∩U, whose restriction to TΣ is positive definite. Write gab0 for its components in the given spacetime chart; its inverse components satisfy g000<0 and the spatial block (g0ij) is positive definite;
  2. gab1 is symmetric and agrees on Σ with the components of ∇ˉ0gab for some smooth extension g of g0 to U;
  3. the harmonic-gauge condition Ha=0 holds on Σ∩U for the pair (g,gˉ) (The harmonic gauge vector, the reduced Einstein equation and the Einstein residual).

Then there is an open neighborhood V⊆U of Σ∩U and a smooth metric g on V with g∣Σ∩U=g0 and ∇ˉ0gab∣Σ∩U=gab1, solving the reduced Einstein equation with the given background gˉ and matter tensor T (The harmonic gauge vector, the reduced Einstein equation and the Einstein residual) on V.

Facts & Assumptions

Given: Countable Choice and the chart and slice, the background metric gˉ, the matter tensor T, and data g0,g1 satisfying conditions 1--3.

[L1]

The reduced Einstein equation is equivalent, on a region where the metric is Lorentzian, g00<0 and (gij) is positive definite, to a first-order quasilinear system for u=(gab,pab=∇ˉ0gab,qabi=∇ˉigab) whose coefficient of the time derivative is the positive definite block matrix diag⁡(I,−g00I,gijI) and whose spatial coefficients are symmetric (Principal part of the reduced Einstein operator and its first-order symmetric hyperbolic reduction clause (b)).

[L2]

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).

[L3]

The data are smooth on the slice, and the metric properties g000<0 and positive definite spatial block persist in a neighborhood of the slice by continuity; a smooth extension of the data to U exists (Cr and smooth maps between smooth manifolds, Smooth covariant 2-tensor fields on a smooth manifold).

Proof

technique · direct
1.1L1L3algebra

(Reduction to a first-order symmetric hyperbolic initial value problem.) Extend g0,g1 to smooth fields on U with gab1=∇ˉ0gab at t=0 [L3], and set pab:=gab1, qabi:=∇ˉigab0 initially. By [L1] the reduced equation, together with the definition of (p,q), is the first-order quasilinear system S(u)=0 on U; at t=0 the time matrix of S is positive definite because g000<0 and (g0ij)>0, and positivity persists in an open neighborhood of the slice by [L3].

2.1step 1.1L2algebra

(Local solution and independence.) Choose a coordinate ball B⋐U meeting Σ∩U and cut off the data and the coefficient functions outside B; the resulting system is a periodic symmetric hyperbolic system after identifying a neighborhood of B with an open subset of T2π3 and extending by constants. By [L2] it has a smooth solution on a time interval around 0; by the finite-speed independence clause of [L2], restricted to the domain of dependence of Σ∩B 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 S(u)=0 on a neighborhood V of Σ∩U.

3.1step 2.1L1algebra∎

(Return to the second-order equation.) The metric equation gives ∇ˉ0g=p. Define the spatial derivative residual Zabi:=qabi−∇ˉigab, initially zero. The transport equation for q contains precisely the commutator Cabi=−Rˉca0igcb−Rˉcb0igac. Subtracting the background derivative identity for ∇ˉig cancels that term and gives a homogeneous linear ODE along each coordinate time line for Z (in component form ∂tZabi=Γˉc0aZcbi+Γˉc0bZaci; the derivative-slot connection terms cancel by background torsion-freeness). Its zero initial value forces Z=0, 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 p=∇ˉ0g and qi=∇ˉig 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 g0,g1 from (h,K) and removes the background dependence by geometric uniqueness, and E3 verifies the matter reductions.

Depends on

Dependency tree · 2 levels

Sources