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Local Einstein-scalar evolution: smooth constrained data admit a local development, unique up to a data-fixing isometry

Statement

Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (ACω), The axiom of dependent choice: a relation in which every element is related to something admits an N-indexed chain). Fix Λ∈R, κ>0 and one scalar model (φ,V,Kϕ) of The scalar-field matter model of the classical gravitational framework, with its fixed smooth potential and normalization. Let Σ be a smooth three-manifold with smooth Riemannian metric h, symmetric tensor K2 and complete scalar data (φ0,π0). Suppose the constraints of Gauss-Codazzi decomposition in Gaussian normal coordinates and the constraint equations in terms of the induced metric and second fundamental form hold for the scalar stress computed from these data, with π0 the prescribed future-normal derivative. Then there is a smooth local Einstein-scalar development Gab+Λgab=κTab,□gφ−V′(φ)=0, with induced geometric data (h,K2), φ∣Σ=φ0 and n(φ)∣Σ=π0. The neighborhood may have position-dependent time width. The initial surface is interior to its intrinsic domain of dependence; restricting to the interior Cauchy neighborhood gives a globally hyperbolic development. Every two developments of this same fixed model and complete data are related near the entire initial surface by a data-fixing time-orientation-preserving isometry matching φ. No potential positivity, mass sign, global existence or uniform noncompact slab is asserted (Local geometric development for a fixed covariant Einstein-matter model with complete constrained data).

Facts & Assumptions

Given: the choice assumptions, fixed constants and scalar model, and the smooth complete constrained data.

[L1]

The scalar supplier gives the actual coupled symmetric-hyperbolic family, complete initialization (φ,P,Q)=(φ0,π0,dφ0), auxiliary recovery and conservation on the reduced metric before Einstein recovery (Symmetric hyperbolic reduction of the Einstein-scalar system and on-shell conservation).

[L2]

The fixed-model development theorem supplies its complete flat harmonic metric initializer, compatible reduced existence, constraint recovery, literal normal-collar gluing, intrinsic Cauchy neighborhood and fixed-data isometry uniqueness (Local geometric development for a fixed covariant Einstein-matter model with complete constrained data). Its flat initial shift derivative includes the contracted spatial Christoffel term; the zero-shift-derivative initializer of Harmonic initial data from geometric data: prescribing the metric jet of a spacelike slice in a time-independent background uses instead comparison metric −dt2+h.

Proof

1.1givenL1L2L3algebra

(Full reduction contract.) Complete scalar data determine every first-order matter variable by [L1], since ∂0=n initially in [L2]'s metric gauge. The supplier verifies the smooth symmetric positive principal matrices and reconstruction of the actual scalar equation on the reduced metric; its conservation identity then makes the reduced stress divergence-free before Einstein recovery. Thus the fixed model and complete data satisfy all reduction, initialization and reduced-conservation hypotheses of [L2]; the constrained stress is exactly [L3].

2.1step 1.1L2∎

(Development and uniqueness.) Apply [L2] with these constrained data. Its reconstructed scalar realizes exactly φ0 and π0, and its full metric realizes h,K2 with the stated equations. Its gluing and causal conclusions give the variable-width solution and intrinsic Cauchy neighborhood, while its uniqueness compares the same potential, normalization and complete data and matches φ by the stated future isometry. No sign assumption beyond the fixed scalar model was introduced.

Remarks

The complete scalar equation is used to obtain conservation. Conservation of the scalar stress alone is not substituted for that equation at critical scalar values.

Depends on

Dependency tree · 2 levels

Sources