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Gr14 Full High Regularity Symmetric Hyperbolic Proof — Examples

1 · Prerequisites

2 · Summary

This page collects worked checks and countermodels for gr-gr14-full-high-regularity-symmetric-hyperbolic-proof.

Constant-coefficient energy method. Worked E0 check: constant-coefficient transport on the three-torus, explicit solution and conserved energy solves the periodic transport system ∂tu+2∂1u=0 explicitly, identifies the solution with the E0 Galerkin limit and verifies the weighted energy identity e′(t)=0.

Sharpness of the torus embedding. The H^1 to C^0 bound fails at s minus m equal to one: dyadic shells have an unbounded C^0/H^1 ratio exhibits the shell functions on T2π3 whose C0/H1 ratio diverges, showing that the hypothesis s−m>3/2 of Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves cannot be relaxed at s−m=1.

Fluid principal symbol. Worked fluid symbol: eigenvalues of the principal matrix for the radiation equation of state at an explicit timelike covector computes the symbol matrix of The barotropic fluid equations in enthalpy form are symmetric hyperbolic with positive principal symbol at a radiation equation of state and evaluates its positive eigenvalues.

Failure without sound-speed positivity in the linearized fluid. A negative pressure derivative defeats fixed-Sobolev evolution: exponentially growing Fourier modes of the linearized barotropic fluid linearizes the fixed-flat-background barotropic equations at a rest state with p′(ϵ0)<0. Its explicit smooth Fourier datum has no periodic classical linearized solution on any positive interval, and its smooth single-mode sequence defeats continuity in every fixed integer Sobolev topology at each positive time. A nonlinear Einstein-fluid result must additionally control the constrained initial data and nonlinear evolution; that transfer remains an open prerequisite.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

CounterexampleConstruction: AI-generatedVerification: AI-generatedprecheck pendingOpen item page →

The H^1 to C^0 bound fails at s minus m equal to one: dyadic shells have an unbounded C^0/H^1 ratio

Statement refuted

Refuted statement: "for s=1 and m=0 on T2π3 (so that s−m=1<32) there is a constant C with ∥u∥C0≤C∥u∥H1 for every u∈H1."

Facts & Assumptions

Given: the torus T2π3, its characters χk, the norms ∥⋅∥H1 and ∥⋅∥C0, and the shell family (uN).

[L1]

Fourier norm formula: for u=∑kakχk with finitely many nonzero coefficients, ∥u∥H12=∑k(1+∣k∣2)∣ak∣2 and ∥u∥C0=sup⁡x∣∑kakχk(x)∣; in particular uN(0)=#{k:2N≤∣k∣<2N+1} for the shell family, whose coefficients are 1 on the shell (Periodic Fourier differentiation identity and equivalence of the derivative and Fourier-weight Sobolev norms, The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s).

[L2]

Lattice-point counts: there are constants 0<c≤C with c23N≤#{k∈Z3:2N≤∣k∣<2N+1}≤C23N for all N≥0 (the shell is a spherical annulus of radius comparable to 2N; each unit cube contains at most one lattice point and volume comparison gives both bounds) (The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s). [L2]

[L3]

In the embedding lemma the hypothesis s−m>3/2 is used exactly at the finiteness of ∑k(1+∣k∣2)−(s−m); at s−m=1 this sum diverges (Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves). [L3]

Counterexample

For N≥0 let uN:=∑k∈Z3, 2N≤∣k∣<2N+1χk. Then ∥uN∥H1≤C25N/2 and uN(0)=∣{k:2N≤∣k∣<2N+1}∣≥c23N for constants c,C>0 independent of N, so the ratio ∥uN∥C0/∥uN∥H1 is at least c′2N/2→∞: no constant C exists, and the identity embedding bound fails at s−m=1. The raw shell norms grow; equivalently, the normalized sequence uN/∥uN∥H1 has unit H1 norm and unbounded C0 norm.

Proof technique: direct.

1.1L1L2algebra

(Norms of the shell family.) By [L1] and [L2]: ∥uN∥H12=∑2N≤∣k∣<2N+1(1+∣k∣2)≤2⋅22N+2⋅#shell≤C22N23N=C25N, so ∥uN∥H1≤C25N/2; and uN(0)=#shell≥c23N.

2.1step 1.1algebra

(Divergence of the ratio.) Hence ∥uN∥C0/∥uN∥H1≥c′23N−5N/2=c′2N/2→∞; if a constant C satisfied the claimed bound, applying it to uN/∥uN∥H1 would give a uniform bound on this ratio, a contradiction.

3.1L3algebra∎

(Consistency with the sharp threshold.) The failure occurs exactly at the exponent where the weight sum of [L3] diverges; by Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves the bound does hold for s−m>3/2, so the counterexample is sharp and does not contradict the embedding theorem.

ExampleConstruction: AI-generatedVerification: AI-generatedprecheck pendingOpen item page →

Worked E0 check: constant-coefficient transport on the three-torus, explicit solution and conserved energy

Example

On T2π3 take m=1, A0=1, A1=2, A2=A3=0, B=0, so the system (⋆) of Periodic first-order symmetric hyperbolic systems: coefficients, admissible values, data classes and solutions reads ∂tu+2∂1u=0, with u0∈Hs real-valued and integer s≥5. This example exhibits the explicit solution on the periodic domain, u(t,x)=u0(x1−2t,x2,x3), verifies that it is the E0 solution, and checks the weighted energy identity e′(t)=0 for the energy e(t)=∫u(t)2 dμ directly.

Facts & Assumptions

Given: the torus data and the system ∂tu+2∂1u=0 with real Hs datum u0, integer s≥5.

[L1]

The periodic torus, its characters and the spaces Hs are those of The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s; for a periodic Hs function the translate x↦u0(x1−2t,x2,x3) is again in Hs with the same norm, by the derivative rule and the periodicity of the Fourier representation (Periodic Fourier differentiation identity and equivalence of the derivative and Fourier-weight Sobolev norms, Periodic Sobolev embedding: H^s on the three-torus controls C^m when s minus m exceeds three halves supplies the C1 representative since s−1>3/2).

[L2]

E0 existence and uniqueness for this system: the data u0 with values in any compact interval and finite Hs norm admit a classical Sobolev solution, unique by Uniqueness of classical solutions and continuous dependence in H^{s-1} for periodic symmetric hyperbolic systems, with ∂tu∈L∞Hs−1; the solution is found by the Galerkin/limit construction (Local existence of Sobolev and classical solutions of a periodic symmetric hyperbolic system, uniform on bounded H^s data). [L2]

[L3]

The metric measure μ is translation invariant on the torus and ∫∂1v dμ=0 for every smooth periodic v (the fundamental theorem of calculus on one period, as in Periodic Fourier differentiation identity and equivalence of the derivative and Fourier-weight Sobolev norms step 1.1). [L3]

[L4]

The finite Fourier projection PN and its range XN are Fourier modes on the periodic three-torus and the Galerkin projection P_N; PN commutes with spatial derivatives and maps Hs into XN (The Galerkin projection is self-adjoint, commutes with derivatives, is a contraction in every H^r, converges to the identity and has the sharp Fourier-tail bound). For A0=1, the weighted Galerkin energy of Equivalence of the weighted Galerkin energy with the H^s norm and its Gronwall inequality is eN(t)=∑∣α∣≤s∥DαuN(t)∥22.

Verification

technique · direct
1.1L1algebra

(The explicit function solves the system.) Define u(t,x):=u0(x1−2t,x2,x3). Then ∂tu(t,x)=−2(∂1u0)(x1−2t,x2,x3) and ∂1u(t,x)=(∂1u0)(x1−2t,x2,x3), so ∂tu+2∂1u=0 pointwise; u(0,⋅)=u0, and u is classical because integer s≥5 and inherits the Hs-bound of u0 at every time, with higher smoothness whenever u0 is smooth.

2.1step 1.1L3algebra

(Energy identity.) e(t)=∫u(t)2dμ=∫u02dμ=e(0) by translation invariance [L3]; equivalently, differentiating under the integral and using the equation and [L3], e′(t)=2∫u∂tu dμ=−4∫u∂1u dμ=−2∫∂1(u2) dμ=0.

3.1step 1.1step 2.1L2L3L4discharge-construct∎

(Identification with the E0 solution.) By [L2] there is a unique solution through u0; the explicit function of step 1.1 is one, so the E0 solution is u(t,x)=u0(x1−2t,x2,x3) and its energy is conserved. For the actual Galerkin energy, set uN(t)=PNu(t), equivalently uN(t,x)=(PNu0)(x1−2t,x2,x3). By [L4] this smooth finite Fourier polynomial solves ∂tuN+2∂1uN=0 with datum PNu0, hence its projected equation. Each Fourier coefficient obeys ∂tu^N(k)=−2ik1u^N(k), so this is exactly the Galerkin trajectory. Every DαuN is the translate of DαPNu0; translation invariance gives eN(t)=∑∣α∣≤s∥DαPNu0∥22=eN(0) and eN′(t)=0. Thus the actual energy inequality is verified with C=0, at every cutoff N, as well as the zero-order identity of step 2.1.

CounterexampleConstruction: AI-generatedVerification: AI-generatedprecheck pendingOpen item page →

A negative pressure derivative defeats fixed-Sobolev evolution: exponentially growing Fourier modes of the linearized barotropic fluid

Statement refuted

Assume Countable Choice ACω (The Axiom of Countable Choice (ACω)), carrying the integration hypothesis of The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s.

Refuted statement: "At every constant rest state with H0=ϵ0+p(ϵ0)>0, the fixed-flat-background linearized barotropic fluid equations admit a periodic C1 solution on some positive time interval for every smooth periodic initial datum, and their solution operators are continuous in each fixed integer Sobolev topology Hr, r≥0, at every fixed positive time."

For p′(ϵ0)=−a2<0, both assertions fail: the explicit smooth datum of step 2.2 has no such solution on any positive time interval, and the smooth single-mode sequence of step 2.1 proves failure of Hr continuity for every integer r≥0 at every fixed positive time. These conclusions concern the specified linearized equations; nonlinear Einstein-fluid illposedness with constrained data remains an open prerequisite.

Facts & Assumptions

Given: Countable Choice, a smooth equation of state near a constant rest density ϵ0 with H0=ϵ0+p(ϵ0)>0 and p′(ϵ0)=−a2<0, the flat metric −dt2+∑i(dxi)2 on R×T2π3, and its rest velocity ∂t. A classical linearized solution means periodic density and spatial velocity perturbations (f,v) of class C1 on [0,τ]×T2π3 satisfying the displayed equations and initial values; derivatives at the time endpoints are one-sided.

[L1]

Perfect-fluid stress and conservation equations are those of The perfect-fluid matter model: rest energy density, pressure, four-velocity and stress-energy; their first variation at the prescribed constant flat rest state is computed directly below.

[L2]

On the fixed flat background the linearization of the system about a constant state with n=∂t, constant ϵ0,p0 decouples the spatial Fourier modes; substituting δϵ=eik⋅xgk(s) into the linearized equations gives gk′′=−p′(ϵ0)∣k∣2gk (The perfect-fluid matter model: rest energy density, pressure, four-velocity and stress-energy). [L2]

[L3]

The normalized measure on T2π3 has total mass one, and for integer r≥0 the Sobolev norm is the derivative-sum norm of The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s, with its declared Countable Choice assumption.

Counterexample

Consider only the fixed-flat-background linearized fluid subsystem at a constant rest state. Write H0=ϵ0+p(ϵ0)>0 and a=−p′(ϵ0)>0. For density perturbation f and spatial velocity perturbation v, differentiation of the conservation equations directly gives ∂tf+H0div⁡v=0,H0∂tv−a2∇f=0. Indeed the normalization equation at the rest state gives δu0=0; the first variations of T00,T0i,Tij are respectively f,H0vi,p′(ϵ0)fδij. These equations therefore follow by ordinary differentiation of the perfect-fluid stress formula, without invoking the real enthalpy reduction, whose hypotheses require p′>0.

The following computation proves both failure of fixed-Sobolev continuity and failure of existence for some smooth data for this linearized system. The nonlinear Einstein-fluid extension remains an open prerequisite: a fixed-flat fluid mode calculation neither solves the nonlinear Einstein constraints nor proves that a merely continuous nonlinear solution map has a bounded derivative. The cited Friedrich--Rendall Section 5.5 makes only the linearized deduction and describes the nonlinear implication as a suggestion. A rigorous nonlinear transfer theorem with constrained initial data, or a direct nonlinear counterexample, is still required here.

Proof technique: direct.

1.1L1L2algebra

(Exact growing and decaying mode solutions.) For every integer n≥1 and A≥0, put fn(t,x)=Acos⁡(nx1)cosh⁡(ant) and vn1(t,x)=−(a/H0)Asin⁡(nx1)sinh⁡(ant), with vn2=vn3=0. Differentiation gives ∂tfn+H0∂1vn1=0 and H0∂tvn1−a2∂1fn=0; the other momentum components are zero. Thus these are exact smooth solutions of the displayed linearized system with data (Acos⁡(nx1),0). The density mode satisfies gn′′=a2n2gn, gn(0)=A, gn′(0)=0, so gn(t)=Acosh⁡(ant)≥(A/2)eant for t≥0. This lower bound uses the stated nonnegative amplitude and zero initial velocity. More generally, for any periodic C1 solution, differentiating its Fourier coefficients under the integral and integrating the spatial derivatives by parts gives gk′=−H0ik⋅wk and H0wk′=a2ikgk, hence gk′′=a2∣k∣2gk. The initial density and velocity therefore determine each density coefficient uniquely by this scalar ODE.

2.1step 1.1L3constructalgebra

(Failure of fixed-Sobolev continuity on smooth modes.) Fix τ>0 and an integer r≥0. In step 1.1 take An=(1+n2)−r/2e−anτ/2. Under the derivative-sum norm of [L3], ∥cos⁡(nx1)∥Hr2=12∑j=0rn2j, which lies between positive constants times (1+n2)r, uniformly for n≥1. Consequently the initial H^r norm tends to zero, whereas the density H^r norm at τ is at least a positive constant times eanτ/2 and tends to infinity. Each datum and solution is a single trigonometric polynomial and hence smooth; indeed the data tend to zero in every fixed derivative norm because exponential decay dominates every power. Any other classical solution of the same datum has the same coefficient at (n,0,0) by step 1.1. For any such density lying in Hr, integration by parts gives nr∣f^(n,0,0)∣=∣D1rf^(n,0,0)∣≤∥D1rf∥2≤∥f∥Hr. The coefficient inequality follows from ∣h^(k)∣≤∫∣h∣≤∥h∥2; the second bound follows by expanding 0≤∫(∣h∣−∫∣h∣)2 on the normalized probability space. Consequently every classical solution choice has density Hr norm at least a positive constant times eanτ/2. Thus no choice of a solution operator, even restricted to these smooth trigonometric data, can be continuous at zero from Hr data to Hr values at any fixed positive time.

2.2step 1.1L2L3constructalgebra

(A genuinely smooth datum with no linearized Sobolev solution.) Set f0(x)=∑n≥1e−ncos⁡(nx1) and v0=0. For every integer q≥0, ∑n≥1nqe−n<∞: group the terms with j2≤n<(j+1)2, whose contribution is at most (2j+1)(j+1)2qe−j, a summable polynomial times a geometric sequence. Thus each spatial derivative series converges uniformly; the fundamental theorem of calculus applied to partial sums and their uniformly convergent derivative series shows successively that f0 is smooth with those derivatives. Suppose a periodic C1 linearized solution existed on [0,τ]. At each Fourier frequency k, differentiation under the integral and periodic integration by parts give gk′=−H0ik⋅wk and H0wk′=a2ikgk. Thus gk is C2 with gk′′=a2∣k∣2gk. The explicit initial coefficients and zero velocity, together with uniqueness of this elementary ODE, force its coefficient at (n,0,0) to be 12e−ncosh⁡(ant). For every t>0 these coefficients tend to infinity, since ant−n→∞, whereas every Fourier coefficient of the continuous density at that fixed time has absolute value at most ∫∣f(t,x)∣ dμ≤sup⁡x∣f(t,x)∣<∞. This contradiction excludes a periodic classical solution on every positive time interval, without requiring an unproved inference from coefficient summability. This explicit datum is smooth; polynomially decaying coefficients of a fixed order would not have established that assertion.

3.1step 2.1step 2.2∎

(Conclusion within the proved scope.) Step 2.1 proves failure of continuity at zero in every fixed integer Hr topology for the explicit smooth mode solutions at each fixed positive time. Step 2.2 supplies one smooth periodic datum admitting no periodic C1 linearized solution on any positive time interval. These refute both assertions in the stated fixed-flat linearized claim. The nonlinear Einstein-fluid transfer with constrained data is explicitly left open; no nonlinear completeness or illposedness verdict follows from this proof.

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Worked fluid symbol: eigenvalues of the principal matrix for the radiation equation of state at an explicit timelike covector

Example

Take the smooth barotropic equation of state p:J→R, J=(0,∞), p(ϵ)=13ϵ, at any state ϵ0∈J. Then ϵ+p=4ϵ/3>0 on J and p′=1/3∈(0,1) (so cs=1/3) and at a point choose a rest frame n with spatial frame (e1,e2,e3) and the future-directed timelike covector ζ=−n♭+12e1♭ (in the notation ζ0=ζ(n)=1, ζ⊥=12e1, so ζ0=1>12=∣ζ⊥∣). This example computes the matrix A(ζ) of The barotropic fluid equations in enthalpy form are symmetric hyperbolic with positive principal symbol and verifies its eigenvalues and positive definiteness explicitly.

Facts & Assumptions

Given: the radiation equation of state on J=(0,∞) and a state ϵ0>0, the rest frame and the covector ζ=−n♭+12e1♭, for which ζ(n)=1 and ζ⊥=12e1♭.

[L1]

The principal symbol of the fluid system in the variables (r,n1,n2,n3) at a covector ζ is the symmetric matrix A(ζ)=(ζ0csζ⊥Tcsζ⊥ζ0I3) (The barotropic fluid equations in enthalpy form are symmetric hyperbolic with positive principal symbol clause (b)).

Verification

technique · direct
1.1L1L2algebra

(The matrix.) By [L1], [L2] and the chosen data, A(ζ)=(11230012310000100001).

2.1step 1.1algebra

(Eigenvalues.) The upper-left block (11231231) has eigenvalues 1±123; the remaining block is the identity with eigenvalue 1 (multiplicity two). All three eigenvalues are positive: 1−123>0 because 23>1.

3.1step 2.1L1algebra∎

(Consistency with the general criterion.) The general criterion of [L1] gives positivity because ζ0=1>12=∣ζ⊥∣ and cs<1; the explicit smallest eigenvalue 1−123≈0.711>0 matches exactly the lower bound ζ0−cs∣ζ⊥∣=1−123 from that criterion.

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