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Local Sobolev stability and continuation for the reduced electrovacuum system
Statement
Assume and the conditional local existence theorem Local high-Sobolev and smooth electrovacuum. Let , let a harmonic-reduced source-free Einstein–Maxwell solution on have first-order state with , and suppose its values stay in a fixed compact admissible state set and . If is finite and lies inside the smooth coefficient-time domain, the reduced solution extends through to a larger interval. If the original state has , , vanishing harmonic vector , and satisfies the full source-free Einstein–Maxwell equations, the extension has these same properties and extends the full development. The same conclusion holds at a finite left endpoint. On every common interval where two reduced solutions have the same fixed harmonic background, compact-state range and uniform bound, their states are unique and satisfy an continuous-dependence estimate.
Facts & Assumptions
Given: Countable Choice, the real componentwise Fourier state and the bounded-state reduced Einstein–Maxwell solution in the Statement.
Local high-Sobolev and smooth electrovacuum gives the full solution regularity, derivative-variable identities, propagation of the Einstein and Maxwell constraints, harmonic gauge, and the Maxwell transport, stress and Einstein subsidiary identities used below. The endpoint is restarted with [L1] in the same reduced state, rather than reinitializing the special lapse/shift jet of that theorem. Its use remains conditional on the CP01 draft carriers recorded there, each of which has precheck pending and is listed in the batch-6 manifest inventory.
Draft supplier Exact periodic positive symmetric-hyperbolic supplier: for integer , smooth periodic symmetric coefficient matrices with uniformly positive time matrix on a compact admissible state neighborhood, and initial data with values in that neighborhood and bounded norm, there is a common local solution with bounds and . Its item file is listed in batch 6; its status is draft and its verification precheck is pending; this input remains conditional.
Uniqueness of classical solutions and continuous dependence in H^{s-1} for periodic symmetric hyperbolic systems proves uniqueness and continuous dependence for classical periodic symmetric-hyperbolic solutions with common compact-state and bounds. Its inspected statement assumes and a common existence interval; its published carrier has precheck pending.
Local existence of Sobolev and classical solutions of a periodic symmetric hyperbolic system, uniform on bounded H^s data gives a common existence interval and for the bounded data class of the preceding supplier. Its published carrier has verification precheck pending.
Periodic high-Sobolev state spaces fixes componentwise. Smooth composition, difference, coefficient product and commutator estimates on bounded H^s data and The periodic Sobolev space H^k of the three-torus is a Banach algebra for k at least four give the coefficient/product bounds on compact state sets, and Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves gives when .
Coupled reduced Einstein–Maxwell local evolution verifies the concrete reduced coefficient family on the open admissible state set: its metric time block is , its Maxwell time block is , every spatial block is symmetric, and all coefficients and lower-order terms are smooth functions of the first-order state and the fixed smooth background. This verification applies to arbitrary admissible reduced states, including endpoint states with nonzero shift; it requires no constraints or special harmonic initial jet.
Proof
By [F5], the reduced equation has the form in the sense of Periodic first-order symmetric hyperbolic systems: coefficients, admissible values, data classes and solutions. Its time matrix is , positive definite throughout the admissible open set. Every spatial matrix is symmetric: the metric wave blocks and the Maxwell curl blocks are symmetric, while the shift adds a scalar identity to the latter. The algebraic stress and the frame derivatives, expressed using , create only smooth zero-order terms, so there is no off-diagonal derivative coupling. Enclose the fixed compact state range in the interior of a larger compact subset of this open set; on that subset and a compact coefficient-time slab containing in its interior, smoothness and strict positivity give bounded coefficient derivatives and a uniform positive time-matrix lower bound. These verify the concrete hypotheses required by [L1] and [F3] at the restart. Since is uniformly bounded and is an algebra for , the equation and [F4] also give near .
For each finite Fourier projection , every coefficient of is absolutely continuous and its derivative is the corresponding coefficient of . Thus . Letting and using Fourier convergence in gives the same estimate for . Hence has a strong limit as .
For each finite frequency set , strong convergence of its coefficients gives where . Taking the supremum over in the Fourier definition [F4] proves and . By the embedding in [F4], uniformly in space. Since each lies in the fixed compact state set, the closedness of that set gives in the same set for every .
For the full-development conclusion, assume the original solution has the compatibility, harmonic and full-equation properties stipulated in the Statement. The derivative identities from [F1] then pass to : because these relations are continuous in the strong limit. Since , the Fourier norm identity gives ; likewise . At the endpoint order needed when , the Fourier convolution estimate and prove ; the same argument with exponent proves the product estimate. The chain rule through order three, , and Fourier approximation give continuity of smooth composition in on compact value sets: first derivatives converge uniformly, higher derivatives converge in , and every chain-rule product therefore converges in . In particular, matrix inversion is continuous in on a compact set of positive-definite metrics. For the supplied algebra/composition estimates at apply directly, and for these local estimates cover the curvature and connection products. The constraints involve at most two spatial derivatives of and one derivative of , which converge in from the first-order state and its derivative identities; each inverse-metric factor and each product in the constraint expressions is thus continuous at the endpoint. The harmonic vector is a smooth function of , so as the limit of . Therefore determines constrained data of precisely the regularity required by [F1].
Restart the same harmonic-reduced coefficient system of [F5] at time with the actual complete state , keeping the fixed background and coordinates unchanged. The coefficients are smooth on the same time-state domain, is interior to its time interval, and step 3.1 supplies an datum with compact admissible range and bounded norm. Applying [L1] (equivalently [F3] after translating time) gives a reduced solution on with . This gives a reduced extension candidate for every state in the Statement, without reinitialization to lapse one, shift zero, or the special metric jet of the original initial slice. For the full-development conclusion, assume now the additional properties used in step 4.1. The reduction's equations propagate by the homogeneous background-commutator ODE, so has the required metric derivative identities. It has the same bounds and compact-state control as the local solver class; the spacetime-regularity argument in proof step 4.1 of [F1], which uses only those bounds, the derivative identities and the fixed smooth coefficients, applies to after translating time and yields and . Its zero initial Maxwell divergence residuals from step 4.1 propagate by the normal-form transport argument of [F1]; the coordinate time foliation is smooth and its normal is at this regularity. Thus both full Maxwell equations hold, and the explicit classical stress identity carried by [F1] gives conservation at the restarted metric/ field regularity; no smooth-only stress theorem is applied. The harmonic residual identity from [F1] gives the homogeneous wave equation for . Initially by step 4.1, so its tangential derivatives vanish. In any orthonormal frame with future unit time vector , the Einstein residual is , hence and there. The endpoint Einstein constraints from step 4.1 give . The same local wave-energy uniqueness argument of [F1], valid for this positive symmetric wave block with bounded coefficient derivatives, yields near the endpoint slice. Therefore is a full solution.
On the overlap before , compare and the old solution using the difference-energy estimate [F2] on with , in the reverse time direction. The compact state sets and norms of both solutions have common bounds, so its constant is uniform as . Their strong traces both tend to , giving . Thus the solutions agree on the overlap, and extends the original reduced solution through , and the full development when the additional hypotheses hold. The same estimate identifies any two continuations. Time reversal gives the left-endpoint case. On each common interval the same [F2] estimate gives the stated continuous dependence, with constants depending on the coefficient time slab, compact state set, norm bound and .
Depends on
The Axiom of Countable Choice ()
Electrovacuum tensor Cauchy system
Periodic high-Sobolev state spaces
Local high-Sobolev and smooth electrovacuum
Coupled reduced Einstein–Maxwell local evolution
Exact periodic positive symmetric-hyperbolic supplier
Periodic first-order symmetric hyperbolic systems: coefficients, admissible values, data classes and solutions
Local existence of Sobolev and classical solutions of a periodic symmetric hyperbolic system, uniform on bounded H^s data
Uniqueness of classical solutions and continuous dependence in H^{s-1} for periodic symmetric hyperbolic systems
Smooth composition, difference, coefficient product and commutator estimates on bounded H^s data
The periodic Sobolev space H^k of the three-torus is a Banach algebra for k at least four
Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves
Dependency tree · 2 levels
Sources
- P. T. Chruściel, An introduction to the Cauchy problem for the Einstein equations, Roscoff lecture notes (2011), §1.6, printed pp. 23–25.
- M. Alcubierre, J. C. Degollado and M. Salgado, The Einstein-Maxwell system in 3+1 form and initial data for multiple charged black holes, arXiv:0907.1151v2 (2009), §II.C, printed pp. 8–9.