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Conformal construction of constrained initial data

1 · Prerequisites

2 · Summary

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

DefinitionDefinition: AI-adaptedProof: AI-generatedprecheck passverified 2026-10-22 (gpt-6.1-sol)Open item page →

Vacuum conformal constraint data

Physical scope

Pure mathematical definition of compact vacuum, zero-cosmological-constant conformal initial data and its algebraic constraint residuals; no embedded development, existence theorem, or empirical claim is asserted.

Definition

Let Σ be a nonempty smooth three-manifold without boundary that is compact: for every family (Ua)a∈A of open subsets of Σ with Σ=⋃a∈AUa, there is a finite subset F⊆A such that Σ=⋃a∈FUa. In this item, “vacuum” means that the stress-energy tensor is zero and the cosmological constant is fixed at Λ=0. Let h~ be a smooth Riemannian metric on Σ, let σ~ be a smooth symmetric covariant two-tensor field, let τ∈R be constant, and let ϕ∈C∞(Σ,R) satisfy ϕ(p)>0 at every p∈Σ. Use the positive scalar ϕ as a dimensionless conformal factor.

Write D~ for the Levi-Civita connection of h~ and D for that of the metric h defined below. On covariant tensor fields, these symbols also denote their induced product connections, with the dual and tensor-factor rules of the product-connection supplier in Definition references. In a chart, h~ij denotes the inverse matrix to h~ij. It is smooth because det⁡(h~ij)>0 and the matrix inverse is the adjugate divided by the determinant. For any smooth Riemannian metric m on Σ, with Levi-Civita connection Dm, define Rm(X,Y)Z:=DXmDYmZ−DYmDXmZ−D[X,Y]mZ. In a chart, R[m]abij denotes the components of Rm(∂i,∂j)∂b. Define Ric⁡(m)ij:=R[m]kikj and R(m):=mijRic⁡(m)ij. In particular, R~:=R(h~), with the same curvature sign convention. Define the scalar Laplacian by Δ~f:=h~ij(∂i∂jf−Γ~kij∂kf), where Γ~kij are the Christoffel symbols of D~, given by the Levi-Civita Christoffel formula in Definition references. The curvature sign is the one displayed above. All traces, norms, raising of indices and contractions in this item use the metric indicated by the subscript. In particular, tr⁡h~σ~:=h~ijσ~ij,∣σ~∣h~2:=h~ikh~jℓσ~ijσ~kℓ,(div⁡h~σ~)j:=h~ikD~iσ~kj. The tensor σ~ is transverse-traceless (TT) with respect to h~ when it is symmetric and both displayed trace and divergence vanish. The input tensor in this definition is required to be TT.

Define h:=ϕ4h~,K:=ϕ−2σ~+τ3h. Because ϕ>0, h is a smooth Riemannian metric; because σ~ and h are symmetric, K is a smooth symmetric tensor. Here h is the candidate induced Riemannian metric and K is the candidate second fundamental form, with the library convention K(X,Y)=g(∇Xn,Y) when the data are induced by a spacelike hypersurface with future unit normal n. The pair is vacuum conformal constraint data. It is abstract data on Σ; no embedding into a spacetime is part of this definition. For its embedded Lorentzian interpretation assume the Axiom of Countable Choice ACω, as in the supplied smooth tangent-bundle convention; the algebraic tensor definitions themselves use no choice principle. Define the h-trace, squared norm and divergence by tr⁡hK:=hijKij,∣K∣h2:=hikhjℓKijKkℓ,(div⁡hK)j:=hikDiKkj. With R(h) computed using h, define the Hamiltonian and momentum residuals H(h,K):=R(h)+(tr⁡hK)2−∣K∣h2,Mj(h,K):=hikDiKkj−Dj(tr⁡hK). The data satisfy the vacuum constraint equations when H(h,K)=0 and M(h,K)=0. For an embedded hypersurface, these are the normal and normal-tangential Einstein constraints in the specified K convention.

Tensoriality of curvature and basis-independent contraction make these scalar curvatures independent of the chart. For dimensional bookkeeping in the SI length convention, [τ]=m−1, [R(h)]=[R~]=[∣σ~∣h~2]=[Δ~]=m−2, and [ϕ]=1. Thus all terms in the scalar constraint equation have units m−2.

Definition references

Facts & Assumptions

Given: A nonempty compact smooth three-manifold, a smooth Riemannian metric h~, a smooth symmetric TT covariant tensor σ~, a positive smooth scalar ϕ, and a constant τ. For the embedded Lorentzian constraint interpretation assume ACω.

[A1]

The Axiom of Countable Choice (ACω), Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model: ACω is the axiom that every countable family of nonempty sets has a choice function; the Lorentzian time-orientation and smooth normal-field conventions use this assumption for the embedded interpretation.

[F1]

Smooth manifolds and their smooth charts, A smooth tensor field: a smooth manifold has smooth coordinate charts, and a smooth tensor field has smooth coordinate components.

[F2]

Riemannian metric and riemannian manifold: a Riemannian metric is a smooth symmetric covariant two-tensor that is positive definite at every point.

[F3]

Fundamental theorem of riemannian geometry: each smooth Riemannian metric has a unique Levi-Civita connection.

[F4]

Integer powers am: negative integer powers are defined for nonzero bases; Laws of integer exponents gives their product and quotient identities.

[F6]

Identity maps and composites of smooth maps are smooth: the composition of smooth maps between smooth manifolds is smooth.

[F7]

Christoffel formula for the levi civita connection: the Christoffel symbols of a smooth Riemannian metric are Γabc=12gad(∂bgdc+∂cgbd−∂dgbc).

[F8]

Curvature is a type (1,3) tensor: the curvature defined from an affine connection is a tensor field of type (1,3).

[F9]

The contraction of a mixed tensor: contraction pairs one covariant and one contravariant slot of a tensor.

[F10]

Contraction is independent of the basis formula: tensor contraction has the same value in every basis.

[F11]

Spacelike initial data, the constraint equations, developments and maximal developments: the library uses K(X,Y)=g(∇Xn,Y) for the second fundamental form, and the vacuum constraints have Λ=0 and vanishing stress-energy.

[F12]

Gauss-Codazzi decomposition in Gaussian normal coordinates and the constraint equations in terms of the induced metric and second fundamental form: in that convention the normal and normal-tangential Einstein projections give the Hamiltonian and momentum constraint residuals.

[F13]

Product connection on tensor and hom bundles: for a smooth function f, its differential is the covector field defined by (df)p(v)=v(f). The induced dual connection on covectors gives (D~idf)j=∂i∂jf−Γ~kij∂kf; contracting this covariant tensor with h~ij is a chart-independent scalar.

Proof

1.1F1F2F3F4F5F6algebra

For each integer n≥1, induction by the product rule gives (tn)′=ntn−1, and the quotient rule on t>0 gives (t−n)′=−nt−n−1; iterating this identity shows that every derivative of t↦t−2 is a constant multiple of a negative integer power, hence is continuous on (0,∞). The map t↦t4 is a polynomial. Thus both maps are smooth there; [F5] gives their Ck regularity at every finite order and [F6] makes their composites with ϕ smooth. Hence h=ϕ4h~ is smooth, symmetric and positive definite, because for every nonzero v∈TpΣ, hp(v,v)=ϕ(p)4h~p(v,v)>0 by [F2]. The same rules show that K=ϕ−2σ~+(τ/3)h is smooth and symmetric. The Riemannian connection theorem [F3] supplies both D~ and D.

2.1F1F3F5F7F8F9F10F13step 1.1algebra

In each chart det⁡(h~ij)>0 and h~ij=adj⁡(h~)ij/det⁡(h~); the adjugate entries are polynomials in the smooth metric components [F1], and the reciprocal is smooth by the same quotient-rule induction as in the earlier proof step 1.1 and finite-order algebra closure [F5]. Thus h~ij is smooth; hij=ϕ−4h~ij is smooth by step 1.1. Formula [F7] therefore makes the Christoffel symbols smooth, so the displayed Laplacian is defined for smooth f. By [F13] it is the trace of the covariant derivative of df, so its value is independent of the chart. By [F8] curvature is tensorial, and by [F9, F10] its Ricci and scalar contractions do not depend on the chart. The same basis-independent contractions define the traces and squared norms; all derivative terms use the connections supplied by [F3].

3.1A1F11F12∎

For data induced by an embedded spacelike hypersurface, the convention in [F11] fixes the sign of K, and [F12] gives precisely the stated Hamiltonian and momentum residuals when Λ=0 and stress-energy vanishes. The abstract data definition itself makes no embedding or development assertion.

TheoremStatement: AI-adaptedProof: AI-generatedprecheck passverified 2026-10-22 (gpt-6.1-sol)Open item page →

Conformal reduction of the vacuum constraint equations

Physical scope

Conditional mathematical identity for smooth compact vacuum conformal data with zero cosmological constant; it proves constraint equivalence only and no existence or spacetime development theorem.

Statement

Let (h,K) be the vacuum conformal constraint data of the definition. Then tr⁡hK=τ and the momentum residual vanishes: Mj(h,K)=0. The Hamiltonian residual is H(h,K)=0⟺−8Δ~ϕ+R~ ϕ−∣σ~∣h~2ϕ−7+23τ2ϕ5=0. The displayed scalar equation is the Lichnerowicz equation for these constant-mean-curvature (CMC) vacuum data. Here CMC means that the trace tr⁡hK is spatially constant; its value is τ.

Statement references

Facts & Assumptions

Given: A nonempty compact smooth three-manifold without boundary, a smooth Riemannian metric h~, a smooth TT covariant two-tensor σ~, a constant τ∈R, and a positive smooth dimensionless function ϕ, with Λ=0 and zero stress-energy. Assume ACω for the embedded Lorentzian constraint interpretation.

[A1]

The Axiom of Countable Choice (ACω), Vacuum conformal constraint data: ACω is the axiom that every countable family of nonempty sets has a choice function; the local definition requires it only for the embedded Lorentzian interpretation, not for the abstract tensor identity.

[F1]

Vacuum conformal constraint data: h=ϕ4h~, K=ϕ−2σ~+(τ/3)h, tr⁡h~σ~=0, D~iσ~ij=0, and Δ~f=h~ij(∂i∂jf−Γ~kij∂kf).

[F2]

Spacelike initial data, the constraint equations, developments and maximal developments: the library initial-data convention is K(X,Y)=g(∇Xn,Y) and the vacuum constraints are the normal and normal-tangential projections with Λ=0 and T=0.

[F3]

Gauss-Codazzi decomposition in Gaussian normal coordinates and the constraint equations in terms of the induced metric and second fundamental form: with this K convention, the vacuum scalar and covector constraint residuals are R(h)+(tr⁡hK)2−∣K∣h2 and div⁡hK−d(tr⁡hK), respectively.

[F4]

Christoffel formula for the levi civita connection: for a smooth Riemannian metric m in coordinates, Γ[m]kij=12mkℓ(∂imjℓ+∂jmiℓ−∂ℓmij).

[F5]

Levi civita connection: a Levi-Civita connection is metric-compatible and torsion-free.

[F6]

Dual connection, Product connection on tensor and hom bundles: the induced covariant derivative on dual and tensor-product bundles obeys the dual-pairing and Leibniz rules, so a metric-compatible connection also annihilates the inverse metric.

[F7]

Clairaut--Schwarz theorem for continuous second partial derivatives: second partial derivatives of a smooth scalar function commute in every coordinate chart.

[F8]

The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a): the derivative of a composite of differentiable Euclidean maps is the composition of their derivatives.

[F11]

Integer powers am, Laws of integer exponents: negative integer powers are reciprocals of positive powers, and integer powers obey the addition and quotient laws on nonzero bases.

Proof

1.1F1algebra

From [F1], hij=ϕ−4h~ij and hijKij=ϕ−6h~ijσ~ij+τ=τ. Writing Aij:=ϕ−2σ~ij, its trace is zero and ∣A∣h2=ϕ−12∣σ~∣h~2: each of the two inverse metrics contributes ϕ−4 and the two A factors contribute ϕ−2. The cross term between A and (τ/3)h vanishes by the trace-free condition, while ∣(τ/3)h∣h2=3(τ/3)2=τ2/3. Hence ∣K∣h2=ϕ−12∣σ~∣h~2+τ23.

1.2F1F4F5F6F7F8F9F10algebra

Put u:=2log⁡ϕ, so h=e2uh~, and let Ckij:=Γ[h]kij−Γ~kij. Substitute hij=e2uh~ij and hij=e−2uh~ij in [F4]; using ∂i(e2uh~jℓ)=e2u(2uih~jℓ+∂ih~jℓ) then gives Ckij=δikuj+δjkui−h~ijuk,ui:=D~iu,uk:=h~kℓuℓ. By the affine-connection Leibniz rule, D∂i(f∂a)=(∂if)∂a+fΓcia∂c. Applying this in the curvature definition [F1] and using [∂i,∂j]=0 gives R[Γ]abij=∂iΓajb−∂jΓaib+ΓaiℓΓℓjb−ΓajℓΓℓib. The difference of two affine connections is tensorial, since the derivative terms in their Leibniz rules cancel. For this type (1,2) tensor, D~iCajb=∂iCajb+Γ~aiℓCℓjb−Γ~ℓijCaℓb−Γ~ℓibCajℓ. Substituting Γ[h]=Γ~+C into the curvature formula, the terms linear in C are D~iCajb−D~jCaib: the two terms containing Γ~ℓij cancel because the lower Christoffel indices are symmetric, and the remaining mixed terms pair with the displayed two covariant-derivative terms. The quadratic terms in C remain, giving R[h]abij=R~abij+D~iCajb−D~jCaib+CaiℓCℓjb−CajℓCℓib. Contracting the output and first direction slots gives Ric⁡(h)ij=Ric⁡~ij+D~kCkij−D~jCkik+CkkℓCℓij−CkjℓCℓik. Directly contracting the displayed C gives D~kCkij=2D~iuj−h~ijΔ~u, Ckik=3ui, and D~jCkik=3D~jui. The two quadratic terms expand to CkkℓCℓij=6uiuj−3h~ij∣du∣h~2 and CkjℓCℓik=5uiuj−2h~ij∣du∣h~2. By [F4] the symbols Γ~kij are symmetric in i,j; hence D~iuj−D~jui=∂i∂ju−∂j∂iu=0 by [F7]. Substitution gives Ric⁡(h)ij=Ric⁡~ij−D~iuj+uiuj−(Δ~u+∣du∣h~2)h~ij. Tracing with hij=ϕ−4h~ij gives R(h)=ϕ−4(R~−4Δ~u−2∣du∣h~2). Since u=2log⁡ϕ, [F8, F9] give ui=2ϕ−1∂iϕ. Differentiating once more by [F10] gives ∂i∂ju=2ϕ−1∂i∂jϕ−2ϕ−2(∂iϕ)(∂jϕ). Substitution in the coordinate Laplacian yields Δ~u=2ϕ−1Δ~ϕ−2ϕ−2∣dϕ∣h~2, with the minus sign applying to the second term. [F8, F9, F10] also give ∣du∣h~2=4ϕ−2∣dϕ∣h~2. The gradient-square terms cancel, so R(h)=ϕ−5(−8Δ~ϕ+R~ ϕ).

2.1F1F3F5F6F8F10F11step 1.2algebra

Raise both indices of Aij with h to get Aij=ϕ−10σ~ij. Apply the tensor-product derivative rule [F6] to A=Akj∂k⊗∂j: (DiA)kj=∂iAkj+Γ[h]kiℓAℓj+Γ[h]jiℓAkℓ, with the same formula for D~. Subtracting cancels the ordinary derivative and gives DiAij=D~iAij+CiikAkj+CjikAik. Metric compatibility [F5, F6] gives Dihkℓ=0 and D~ih~kℓ=0: apply the dual-pairing rule to hkℓhℓm=δmk and use Dh=0 (and likewise for h~). The chain and quotient rules give ∂iϕ−1=−ϕ−2∂iϕ; applying the product rule to ten factors and using [F11] gives ∂iϕ−10=10ϕ−9(−ϕ−2∂iϕ)=−10ϕ−11∂iϕ. Now Ciik=6ϕ−1∂kϕ, and, because σ~ is symmetric and trace-free, Cjikσ~ik=4ϕ−1∂iϕ σ~ij; D~i(ϕ−10σ~ij) contributes −10ϕ−11∂iϕ σ~ij+ϕ−10D~iσ~ij, so the three conformal gradient terms cancel. By metric compatibility and the TT condition, D~iσ~ij=h~jℓh~ikD~iσ~kℓ=h~jℓ(div⁡h~σ~)ℓ=0. Therefore DiAij=0. Lowering the free index with the metric-compatible connection gives hjℓDiAiℓ=Di(hjℓAiℓ)=DiAij=hikDiAkj=0, so div⁡hA=0. The pure trace part contributes hikDi((τ/3)hkj)−Djτ=0, because Dh=0 by [F5, F6] and τ is constant by [F1]. Therefore M(h,K)=0.

3.1A1F1F2F3step 1.1step 1.2step 2.1algebra∎

By [F3] and steps 1.1 and 1.2, H(h,K)=ϕ−5(−8Δ~ϕ+R~ ϕ)+23τ2−ϕ−12∣σ~∣h~2. Multiplying by ϕ5>0 is reversible and gives exactly the scalar equation in the Statement. The momentum residual is already zero by step 2.1, so simultaneous satisfaction of both vacuum constraints is equivalent to that scalar equation. This is a deduction about the constraint equations only; it does not assert a solution of the nonlinear equation for arbitrary free data.

Remarks

The conformal weight is attached to the covariant TT tensor σ~ij: after raising both indices with h, its weight is ϕ−10, and its one-index divergence is ϕ−6D~iσ~ij. No general Yamabe, non-CMC, puncture, matter, or conformal-thin-sandwich existence claim follows.

PropositionStatement: AI-adaptedProof: AI-generatedprecheck passverified 2026-10-22 (gpt-6.1-sol)Open item page →

Exact positive constant solution of the CMC constraint equation

Physical scope

Exact algebraic solution of the zero-cosmological-constant CMC vacuum constraint equation in the stated constant-coefficient case; it is not a universal solvability theorem.

Statement

Let the vacuum conformal data be as in the definition, so that σ~ is TT with respect to h~. Suppose the conformal metric has R~=0 and ∣σ~∣h~2=A is a positive constant, with constant τ≠0. Then the Lichnerowicz equation has exactly one positive constant solution, ϕ0=(3A2τ2)1/12. With a fixed length unit, [A]=[τ2]=m−2, so ϕ0 is dimensionless. Uniqueness is only among positive constant solutions; no uniqueness claim is made for arbitrary positive functions.

Facts & Assumptions

Given: Vacuum conformal data as in the definition, including a smooth TT covariant tensor σ~ on a nonempty compact smooth three-manifold, with R~=0, ∣σ~∣h~2=A>0, and constant τ≠0. Assume ACω for the inherited embedded Lorentzian constraint interpretation.

[A1]

The Axiom of Countable Choice (ACω), Vacuum conformal constraint data: ACω is the axiom that every countable family of nonempty sets has a choice function; the local definition requires it only for an embedded Lorentzian interpretation, not for this algebraic solution.

[F1]

Vacuum conformal constraint data: ϕ is positive and dimensionless, τ is the constant trace parameter, and the zero-Λ vacuum scalar residual is defined using R~ and ∣σ~∣h~2; the input σ~ is symmetric, trace-free and divergence-free with respect to h~.

[F2]

Conformal reduction of the vacuum constraint equations: the scalar residual vanishes exactly when −8Δ~ϕ+R~ϕ−∣σ~∣h~2ϕ−7+(2/3)τ2ϕ5=0.

[F3]

Existence and uniqueness of n-th roots: a unique a1/n≥0 with (a1/n)n=a: every positive real number has a unique positive twelfth root.

[F4]

Rational powers ar of a positive base: for a positive base, x1/12 denotes its unique positive twelfth root.

Proof

1.1A1F1F2algebra

For a constant ϕ>0, Δ~ϕ=0. Substituting R~=0 and ∣σ~∣h~2=A in [F2], its equation becomes −Aϕ−7+(2/3)τ2ϕ5=0. Multiplication by ϕ7>0 is reversible, so this is equivalent to ϕ12=3A/(2τ2).

2.1F3F4step 1.1algebra∎

The right side 3A/(2τ2) is positive because A>0 and τ≠0. By [F3], it has exactly one positive twelfth root, and by [F4] that root is (3A/(2τ2))1/12. Thus this is the unique positive constant solution.

Remarks

This is an exact algebraic solution for the stated constant seed data. It does not establish solvability for other conformal metrics or TT tensors.

PropositionStatement: AI-adaptedProof: AI-generatedprecheck passverified 2026-10-22 (gpt-6.1-sol)Open item page →

Positive Fourier inverse for the linearized CMC constraint

Physical scope

Fourier analysis of the linearized vacuum CMC constraint operator at the stated flat-torus solution; it proves a positive linear inverse and no nonlinear nearby-data existence theorem.

Statement

Let Σ=T2π3 with dimensionless coordinates xi(mod2π) and flat conformal metric h~=L∗2∑i=13(dxi)2, where L∗>0 is a fixed reference length. Suppose σ~ has constant squared norm A>0 and τ≠0, and let ϕ0 be the positive constant solution in the preceding proposition. Put c:=7Aϕ0−8+103τ2ϕ04>0. The directional linearization of the Lichnerowicz scalar expression at ϕ0 is Av=−8Δ~v+cv. It is strictly positive on nonzero smooth real v. For every integer s≥2, the same differential expression, interpreted using weak derivatives, defines a bounded bijection A:Hs+2(T2π3)→Hs(T2π3). With Fourier coefficients relative to the normalized torus measure, its inverse is A−1f^(k)=f^(k)8L∗−2∣k∣2+c,k∈Z3, and, for Ns(f)2:=∑k(1+∣k∣2)s∣f^(k)∣2, Ns+2(A−1f)≤min⁡{8L∗−2,c}−1Ns(f). The equivalent derivative Sobolev norms therefore give a bounded Hs→Hs+2 inverse. This linear result does not assert nonlinear differentiability of the constraint map or nearby-data solvability.

Statement references

Facts & Assumptions

Given: The flat torus with L∗>0, constant A>0 and τ≠0, and ϕ0>0 as in the preceding proposition. Assume ACω for the Fourier Sobolev suppliers and inherited embedded Lorentzian interpretation. Let χk([x])=eik⋅x and f^(k)=∫fχk‾ dμ use the normalized measure μ of the torus supplier.

[A1]

The Axiom of Countable Choice (ACω), Vacuum conformal constraint data, The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s, Periodic Fourier differentiation identity and equivalence of the derivative and Fourier-weight Sobolev norms: ACω is the axiom that every countable family of nonempty sets has a choice function; the Fourier Sobolev suppliers state it explicitly, and the local GR definition carries it only for embedded interpretation.

[F1]

Vacuum conformal constraint data: ϕ is positive and dimensionless; the metric's Christoffel symbols use the Levi-Civita formula, curvature is computed from that connection, and Δ~ is its metric Laplacian.

[F2]

Conformal reduction of the vacuum constraint equations: the scalar expression is C(ϕ)=−8Δ~ϕ+R~ϕ−∣σ~∣h~2ϕ−7+(2/3)τ2ϕ5.

[F3]

Exact positive constant solution of the CMC constraint equation: ϕ0>0 solves this equation for the stated flat constant seed data.

[F4]

The 2 pi-periodic three-torus, its normalized measure, test functions and the Sobolev spaces H^s: the torus is R3/(2πZ)3, smooth functions lift to smooth periodic functions, its normalized measure is Lebesgue measure on a fundamental cube divided by (2π)3, its characters are indexed by k∈Z3, and Hs is defined by weak derivatives.

[F5]

Periodic Fourier differentiation identity and equivalence of the derivative and Fourier-weight Sobolev norms: the Fourier differentiation identity holds and Ns is equivalent to the derivative Sobolev norm for every nonnegative integer s.

[F6]

The Fourier basis and Parseval's identity on the finite torus: the Fourier coefficient map is a surjective isometry from complex L2 onto ℓ2(Z3); real-valued inputs have conjugate-symmetric coefficients.

[F8]

A continuous real-valued function on a nonempty compact metric space is bounded and attains a greatest and a least value: every continuous real-valued function on a nonempty compact metric space is bounded and attains its extrema.

Proof

1.1A1F1F2F3F4F7F8algebra

For a fixed smooth real direction v, its periodic lift is continuous on the nonempty compact box [0,2π]3 by [F4, F7], so [F8] gives a finite bound V:=sup⁡∣v∣. If V>0, choose ∣ϵ∣<ϕ0/(2V); if V=0, positivity is immediate. In either case ϕ0+ϵv>0 for all such directions and sufficiently small ∣ϵ∣. Every term in c is positive because A>0, ϕ0>0 and τ≠0. Since h~ij=L∗2δij, the Christoffel formula in the conformal-data definition gives Γ~kij=0 in the local periodic charts. The curvature definition then gives R~=0, and the Laplacian formula gives Δ~=L∗−2∑i∂i2. Differentiating the scalar expression [F2] at the constant ϕ0 gives −8Δ~v from its linear Laplacian term, zero from R~=0, 7Aϕ0−8v from −Aϕ−7, and (10/3)τ2ϕ04v from (2/3)τ2ϕ5. Thus its directional linearization is A=−8Δ~+c. For each i, periodicity makes the integral of ∂i(v∂iv) over one period zero; expanding that derivative gives ∫v∂i2v dμ=−∫(∂iv)2 dμ. Summing over i therefore yields ∫vAv dμ=8L∗−2∫∣∇0v∣2 dμ+c∫v2 dμ>0 for every nonzero smooth real v: choose a point where v≠0; continuity gives a coordinate box of positive torus measure on which ∣v∣ is bounded below by a positive constant, so ∫v2dμ>0. Here ∇0v=(∂1v,∂2v,∂3v).

2.1F4F5F6step 1.1algebra∎

For any v∈Hs+2, the weak-derivative Fourier identity [F5] gives Av^(k)=akv^(k) with ak=8L∗−2∣k∣2+c. Since c>0, every ak>0, and ak≥m(1+∣k∣2) for m:=min⁡{8L∗−2,c}>0; also ak≤M(1+∣k∣2) for M:=max⁡{8L∗−2,c}. The upper bound proves Ns(Av)≤MNs+2(v). Norm equivalence in [F5] therefore makes the weak operator bounded for the derivative Sobolev norms. For real f∈Hs, [F6] gives f^(−k)=f^(k)‾. Since a−k=ak is real, v^(k):=f^(k)/ak has the same conjugate symmetry and therefore [F6] gives it a unique complex L2 representative v. The coefficient definition gives v‾^(k)=v^(−k)‾=v^(k), so injectivity of the coefficient isometry [F6] yields v‾=v in L2. The lower bound gives Ns+2(v)2=∑k(1+∣k∣2)s+2ak2∣f^(k)∣2≤m−2Ns(f)2. The lower bound makes the coefficient sequence square-summable with weight (1+∣k∣2)s+2; [F5] then gives v∈Hs+2, with Av=f. If Av=0, then akv^(k)=0 for every k, hence all coefficients vanish and v=0. This proves surjectivity, injectivity and the asserted inverse bound for every integer s≥2.

Remarks

The zero Fourier mode is invertible because a0=c>0. The result supplies the linear inverse only; a nonlinear implicit-function argument would also require an explicitly proved positive-open domain and composition estimates.

5 · Examples, experiments and counterexamples

None yet.

Sources