The moment-Hessian inequality, its operator data, and $\CPaff\le\CMH$
Part of the moment-map mechanism, Chapter The moment map: CMH and the linear test ; the reading order is on the full proofs page.
Overview. This dossier fixes the operator data of Route C, which answers Remark 15.2 . It proves the Bochner identity Proposition 16.1 , the endpoint reduction Theorem 16.1 (C P a f f ≤ C C M H \CPaff\le\CMH C P aff ≤ C CMH ), the Hodge decomposition Proposition 16.2 with its consequence Corollary 16.1 , and the algebraic countermodel Proposition 16.3 . The work is done in the regular moment-map class. The reduction is a spectral duality argument. C M H ( 4 ) \mathrm{CMH}(4) CMH ( 4 ) itself is not proved, and neither is a strict nonimplication between CMH and KLS. The passage beyond the regular class is only a conditional template, deferred to Proposition 15.1 .
The Stein identity div μ H = − p \Div_\mu H=-p div μ H = − p makes L μ L_\mu L μ symmetric and nonpositive with Dirichlet form E ⟨ H ∇ f , ∇ g ⟩ \E\inner{H\nabla f}{\nabla g} E ⟨ H ∇ f , ∇ g ⟩ (Lemma D30.1 ).
Bochner identity: E ( L μ g ) 2 = E [ ⟨ H ∇ g , ∇ g ⟩ + Tr ( H D 2 g H D 2 g ) ] \E(L_\mu g)^2=\E[\inner{H\nabla g}{\nabla g}+\Tr(HD^2gHD^2g)] E ( L μ g ) 2 = E [ ⟨ H ∇ g , ∇ g ⟩ + Tr ( H D 2 g H D 2 g )] . It uses the total symmetry (D30.5) of the moment map (Proposition D30.1 ) and is not needed for step 3.
Endpoint: pairing f f f with the spectrally truncated A − 1 f \Aop^{-1}f A − 1 f and applying Cauchy–Schwarz gives C P a f f ≤ C C M H \CPaff\le\CMH C P aff ≤ C CMH (Theorem D30.1 ). This uses only step 1.
Hodge: H ∇ g H\nabla g H ∇ g splits orthogonally into Σ ∇ A 1 − 1 h \Sigma\nabla\Aop_1^{-1}h Σ∇ A 1 − 1 h and a divergence-free w w w (Proposition D30.2 ), using (D30.13) . The first channel is exactly C P a f f \CPaff C P aff , and w w w is the only possible gap (Corollary D30.1 ).
Linear test functions show that C M H ( 4 ) \mathrm{CMH}(4) CMH ( 4 ) implies gate zero. Lemma D30.2 isolates the commutator. An explicit random H ⪰ 0 H\succeq0 H ⪰ 0 with E H = I d \E H=\Id E H = Id satisfies the Letwin matrix bound but has λ max ( E H 2 ) > 4 \lmax(\E H^2)>4 λ m a x ( E H 2 ) > 4 for m ≥ 18 m\ge18 m ≥ 18 (Proposition D30.3 ). It is not claimed to be a moment-map Hessian, so Conjecture 16.1 is not refuted (Corollary D30.2 ).
Scope. This dossier discharges Remark 15.2 of Chapter The moment map: the deterministic inequality : it fixes every operator datum in the schematic Route C endpoint ∥ Σ − 1 / 2 H ∇ g ∥ 2 2 ≤ 4 ∥ − L g ∥ 2 2 \norm{\Sigma^{-1/2}H\nabla g}_2^2\le4\norm{-Lg}_2^2 ∥ ∥ Σ − 1/2 H ∇ g ∥ ∥ 2 2 ≤ 4 ∥ − Lg ∥ 2 2 and proves the reduction to the affine Poincaré inequality. It then proves two structural facts about the resulting statement: that it dominates the affine Poincaré constant and has an additional solenoidal channel in dimension at least two (without proving a strict nonimplication), and that its linear-sector consequence is not implied by Letwin’s constant-matrix estimate through matrix algebra alone. It does not prove C M H ( 4 ) \mathrm{CMH}(4) CMH ( 4 ) , which remains open (Conjecture 16.1 is only its necessary linear sector).
Standing hypotheses. μ \mu μ is a centered, full-dimensional log-concave probability measure on R n \R^n R n with density ρ = e − V / Z \rho=e^{-V}/Z ρ = e − V / Z and covariance Σ = Cov μ ≻ 0 \Sigma=\Cov_\mu\succ0 Σ = Cov μ ≻ 0 , lying in the regular moment-map class of §Moment-map coordinates : the moment potential φ \varphi φ of (4.1) is smooth and strictly convex, ∇ φ \nabla\varphi ∇ φ is a diffeomorphism, and the integrations by parts below are justified for compactly supported fields or fields of vanishing normal flux, the general case following by completion. H H H is the moment-map Hessian in target coordinates (4.19) , so that H = H ⊤ ≻ 0 H=H^\top\succ0 H = H ⊤ ≻ 0 , div μ H = − p \Div_\mu H=-p div μ H = − p , and E μ H = Σ \E_\mu H=\Sigma E μ H = Σ . The final paragraph records a conditional limiting template. Existence of approximants with all the required uniformity, affine-support control, and limiting core density is the separate open Proposition 15.1 , not a theorem of this dossier.
1. The operator data ¶ Define the Stein generator and its nonnegative form
L μ g = div μ ( H ∇ g ) = Tr ( H D 2 g ) − p ⋅ ∇ g , A = − L μ , div μ u = ρ − 1 div ( ρ u ) . L_\mu g=\Div_\mu(H\nabla g)=\Tr(HD^2g)-p\cdot\nabla g,
\qquad \Aop=-L_\mu,
\qquad \Div_\mu u=\rho^{-1}\Div(\rho u). L μ g = div μ ( H ∇ g ) = Tr ( H D 2 g ) − p ⋅ ∇ g , A = − L μ , div μ u = ρ − 1 div ( ρ u ) . For f , g f,g f , g smooth with the flux convention above, − E μ [ f L μ g ] = E μ ⟨ H ∇ f , ∇ g ⟩ -\E_\mu[fL_\mu g]=\E_\mu\inner{H\nabla f}{\nabla g} − E μ [ f L μ g ] = E μ ⟨ H ∇ f , ∇ g ⟩ . In particular L μ L_\mu L μ is symmetric and nonpositive on L 2 ( μ ) L^2(\mu) L 2 ( μ ) , the form E H ( f , g ) = E μ ⟨ H ∇ f , ∇ g ⟩ \calE_H(f,g)=\E_\mu\inner{H\nabla f}{\nabla g} E H ( f , g ) = E μ ⟨ H ∇ f , ∇ g ⟩ is closable, and A \Aop A is its nonnegative self-adjoint operator.
E μ [ f L μ g ] = ∫ f div ( ρ H ∇ g ) = − ∫ ρ ⟨ H ∇ f , ∇ g ⟩ \E_\mu[fL_\mu g]=\int f\Div(\rho H\nabla g)=-\int\rho\inner{H\nabla f}{\nabla g} E μ [ f L μ g ] = ∫ f div ( ρ H ∇ g ) = − ∫ ρ ⟨ H ∇ f , ∇ g ⟩ by the divergence theorem and the vanishing flux. Symmetry and nonpositivity follow from H = H ⊤ H=H^\top H = H ⊤ and H ≻ 0 H\succ0 H ≻ 0 ; closability of a densely defined nonnegative symmetric form with smooth positive coefficients is standard.
That the same measure μ \mu μ appears in the form and in the generator is exactly the Stein identity div μ H = − p \Div_\mu H=-p div μ H = − p ; this is what makes Definition 16.1 canonical rather than a choice of reference measure.
C C M H ( μ ) \CMH(\mu) C CMH ( μ ) is defined by (16.5) , with L 2 = L 2 ( μ ) L^2=L^2(\mu) L 2 = L 2 ( μ ) , admissible class Dom ( A ) ∖ ker A \Dom(\Aop)\setminus\ker\Aop Dom ( A ) ∖ ker A , and every inverse the pseudoinverse on ( ker A ) ⊥ (\ker\Aop)^\perp ( ker A ) ⊥ . For μ \mu μ supported on a proper affine subspace, Σ − 1 \Sigma^{-1} Σ − 1 is the inverse on the affine tangent space, equivalently the Moore–Penrose inverse in ambient coordinates.
2. The Bochner identity ¶ For g g g in the core, E μ ( L μ g ) 2 = E μ [ ⟨ H ∇ g , ∇ g ⟩ + Tr ( H D 2 g H D 2 g ) ] \E_\mu(L_\mu g)^2=\E_\mu\bigl[\inner{H\nabla g}{\nabla g}+\Tr(HD^2g\,HD^2g)\bigr] E μ ( L μ g ) 2 = E μ [ ⟨ H ∇ g , ∇ g ⟩ + Tr ( H D 2 g H D 2 g ) ] .
We calculate in target coordinates, use Einstein summation, and first take g g g in a smooth compactly supported core. The Stein identity and the generator formula are
∂ i ( ρ H i j ) = − ρ p j , L μ g = H k ℓ g k ℓ − p k g k . \partial_i(\rho H_{ij})=-\rho p_j,
\qquad L_\mu g=H_{k\ell}g_{k\ell}-p_k g_k. ∂ i ( ρ H ij ) = − ρ p j , L μ g = H k ℓ g k ℓ − p k g k . Integrating once and differentiating L μ g L_\mu g L μ g gives
E μ ( L μ g ) 2 = E μ [ H i j g i g j ] − E μ [ H i j g j ( ∂ i H k ℓ ) g k ℓ ] − E μ [ H i j g j H k ℓ g i k ℓ ] + E μ [ H i j g j p k g i k ] . \begin{aligned}
\E_\mu(L_\mu g)^2
={}&\E_\mu[H_{ij}g_i g_j]
-\E_\mu[H_{ij}g_j(\partial_iH_{k\ell})g_{k\ell}]\\
&-\E_\mu[H_{ij}g_jH_{k\ell}g_{ik\ell}]
+\E_\mu[H_{ij}g_jp_k g_{ik}].
\end{aligned} E μ ( L μ g ) 2 = E μ [ H ij g i g j ] − E μ [ H ij g j ( ∂ i H k ℓ ) g k ℓ ] − E μ [ H ij g j H k ℓ g ik ℓ ] + E μ [ H ij g j p k g ik ] . Integrating the third-derivative term in p k p_k p k gives
− E μ [ H i j g j H k ℓ g i k ℓ ] = − E μ [ p ℓ H i j g j g i ℓ ] + E μ [ H k ℓ ( ∂ k H i j ) g j g i ℓ ] + E μ [ H k ℓ H i j g j k g i ℓ ] . \begin{aligned}
-\E_\mu[H_{ij}g_jH_{k\ell}g_{ik\ell}]
={}&-\E_\mu[p_\ell H_{ij}g_jg_{i\ell}]
+\E_\mu[H_{k\ell}(\partial_kH_{ij})g_jg_{i\ell}]\\
&+\E_\mu[H_{k\ell}H_{ij}g_{jk}g_{i\ell}].
\end{aligned} − E μ [ H ij g j H k ℓ g ik ℓ ] = − E μ [ p ℓ H ij g j g i ℓ ] + E μ [ H k ℓ ( ∂ k H ij ) g j g i ℓ ] + E μ [ H k ℓ H ij g jk g i ℓ ] . The first term on the right cancels the preceding p k p_k p k term after relabelling, and the last one is Tr ( H D 2 g H D 2 g ) \Tr(HD^2g\,HD^2g) Tr ( H D 2 g H D 2 g ) .
The remaining cancellation is exactly where the moment-map structure enters. If p = ∇ φ ( y ) p=\nabla\varphi(y) p = ∇ φ ( y ) and H k ℓ ( p ) = φ k ℓ ( y ) H_{k\ell}(p)=\varphi_{k\ell}(y) H k ℓ ( p ) = φ k ℓ ( y ) , then
H m j ∂ j H k ℓ = H m j ( H − 1 ) r j φ k ℓ r = φ m k ℓ , H_{mj}\partial_jH_{k\ell}
=H_{mj}(H^{-1})_{rj}\varphi_{k\ell r}
=\varphi_{mk\ell}, H mj ∂ j H k ℓ = H mj ( H − 1 ) r j φ k ℓ r = φ mk ℓ , which is totally symmetric in m , k , ℓ m,k,\ell m , k , ℓ . Hence the two residual terms are
E μ [ g j g i ℓ φ ℓ i j ] − E μ [ g j g k ℓ φ j k ℓ ] = 0. \E_\mu[g_jg_{i\ell}\varphi_{\ell ij}]
-\E_\mu[g_jg_{k\ell}\varphi_{jk\ell}]=0. E μ [ g j g i ℓ φ ℓ ij ] − E μ [ g j g k ℓ φ jk ℓ ] = 0. This proves the identity on the smooth core. If g q g_q g q is graph-norm Cauchy there, apply the identity to g q − g r g_q-g_r g q − g r . Since its two right-hand terms are nonnegative, H 1 / 2 ∇ g q H^{1/2}\nabla g_q H 1/2 ∇ g q and H 1 / 2 D 2 g q H 1 / 2 H^{1/2}D^2g_qH^{1/2} H 1/2 D 2 g q H 1/2 are Cauchy in their respective L 2 L^2 L 2 spaces. Their limits define the closed right-hand side, and passage to the limit proves the identity on the operator-core closure.
For μ \mu μ Gaussian, H = I d H=\Id H = Id and the proposition specializes to the familiar Ornstein–Uhlenbeck identity E ( L g ) 2 = E [ ∣ ∇ g ∣ 2 + ∥ D 2 g ∥ H S 2 ] \E(Lg)^2=\E[\abs{\nabla g}^2+\norm{D^2g}_{\HS}^2] E ( Lg ) 2 = E [ ∣ ∇ g ∣ 2 + ∥ ∥ D 2 g ∥ ∥ HS 2 ] . This is a calibration of the formula; the proof above is analytic and uses no numerical evidence.
Proposition D30.1 is not used in the endpoint reduction below. It is recorded because it exhibits the CMH denominator as a sum of two nonnegative pieces, which is what makes the pointwise criterion C C M H ≤ ess sup λ max ( Σ − 1 / 2 H Σ − 1 / 2 ) \CMH\le\operatorname*{ess\,sup}\lmax(\Sigma^{-1/2}H\Sigma^{-1/2}) C CMH ≤ ess sup λ m a x ( Σ − 1/2 H Σ − 1/2 ) available. The total symmetry in (D30.5) is the only place moment-map structure enters. For a general positive symmetric Stein kernel the same calculation leaves an additional ∂ H \partial H ∂ H term with no prescribed sign, so neither this equality nor a one-sided replacement follows from the Stein identity alone.
3. The endpoint reduction ¶ C P a f f ( μ ) ≤ C C M H ( μ ) \CPaff(\mu)\le\CMH(\mu) C P aff ( μ ) ≤ C CMH ( μ ) . In particular C M H ( C ) \mathrm{CMH}(C) CMH ( C ) implies Var μ f ≤ C E μ ⟨ Σ ∇ f , ∇ f ⟩ \Var_\mu f\le C\,\E_\mu\inner{\Sigma\nabla f}{\nabla f} Var μ f ≤ C E μ ⟨ Σ∇ f , ∇ f ⟩ for every f ∈ H 1 ( μ ) f\in H^1(\mu) f ∈ H 1 ( μ ) .
Write C = C C M H ( μ ) C=\CMH(\mu) C = C CMH ( μ ) ; the assertion is automatic if C = ∞ C=\infty C = ∞ . Let C \mathscr C C be the restrictions to supp μ \operatorname{supp}\mu supp μ of R + C c ∞ ( R n ) \R+C_c^\infty(\R^n) R + C c ∞ ( R n ) and first take a centered f ∈ C f\in\mathscr C f ∈ C . This class lies in both form domains even when H H H is globally unbounded: the Stein normalization E μ H = Σ \E_\mu H=\Sigma E μ H = Σ gives
E μ ⟨ H ∇ f , ∇ f ⟩ ≤ ∥ ∇ f ∥ ∞ 2 E μ Tr H = ∥ ∇ f ∥ ∞ 2 Tr Σ < ∞ . \E_\mu\inner{H\nabla f}{\nabla f}
\le \norm{\nabla f}_\infty^2\E_\mu\Tr H
=\norm{\nabla f}_\infty^2\Tr\Sigma<\infty. E μ ⟨ H ∇ f , ∇ f ⟩ ≤ ∥ ∇ f ∥ ∞ 2 E μ Tr H = ∥ ∇ f ∥ ∞ 2 Tr Σ < ∞. For 0 < ε < R < ∞ 0<\eps<R<\infty 0 < ε < R < ∞ put
Π ε , R = 1 [ ε , R ] ( A ) , g ε , R = Π ε , R A − 1 f ∈ Dom ( A ) . \Pi_{\eps,R}=\one_{[\eps,R]}(\Aop),
\qquad g_{\eps,R}=\Pi_{\eps,R}\Aop^{-1}f\in\Dom(\Aop). Π ε , R = 1 [ ε , R ] ( A ) , g ε , R = Π ε , R A − 1 f ∈ Dom ( A ) . Then A g ε , R = Π ε , R f \Aop g_{\eps,R}=\Pi_{\eps,R}f A g ε , R = Π ε , R f . Since f f f is in the H H H -form domain and g ε , R ∈ Dom ( A ) g_{\eps,R}\in\Dom(\Aop) g ε , R ∈ Dom ( A ) , the form–operator pairing and Lemma D30.1 give
∥ Π ε , R f ∥ 2 2 = ⟨ f , Π ε , R f ⟩ L 2 = ⟨ f , A g ε , R ⟩ L 2 = E μ ⟨ ∇ f , H ∇ g ε , R ⟩ ≤ ( E μ ⟨ Σ ∇ f , ∇ f ⟩ ) 1 / 2 ( E μ ⟨ H ∇ g ε , R , Σ − 1 H ∇ g ε , R ⟩ ) 1 / 2 ≤ C 1 / 2 ( E μ ⟨ Σ ∇ f , ∇ f ⟩ ) 1 / 2 ∥ Π ε , R f ∥ 2 . \begin{aligned}
\norm{\Pi_{\eps,R}f}_2^2
&=\inner{f}{\Pi_{\eps,R}f}_{L^2}
=\inner{f}{\Aop g_{\eps,R}}_{L^2}
=\E_\mu\inner{\nabla f}{H\nabla g_{\eps,R}}\\
&\le\Bigl(\E_\mu\inner{\Sigma\nabla f}{\nabla f}\Bigr)^{1/2}
\Bigl(\E_\mu\inner{H\nabla g_{\eps,R}}
{\Sigma^{-1}H\nabla g_{\eps,R}}\Bigr)^{1/2}\\
&\le C^{1/2}
\Bigl(\E_\mu\inner{\Sigma\nabla f}{\nabla f}\Bigr)^{1/2}
\norm{\Pi_{\eps,R}f}_2.
\end{aligned} ∥ Π ε , R f ∥ 2 2 = ⟨ f , Π ε , R f ⟩ L 2 = ⟨ f , A g ε , R ⟩ L 2 = E μ ⟨ ∇ f , H ∇ g ε , R ⟩ ≤ ( E μ ⟨ Σ∇ f , ∇ f ⟩ ) 1/2 ( E μ ⟨ H ∇ g ε , R , Σ − 1 H ∇ g ε , R ⟩ ) 1/2 ≤ C 1/2 ( E μ ⟨ Σ∇ f , ∇ f ⟩ ) 1/2 ∥ Π ε , R f ∥ 2 . After division (unless the projected norm is zero, when the conclusion is immediate) and squaring,
∥ Π ε , R f ∥ 2 2 ≤ C E μ ⟨ Σ ∇ f , ∇ f ⟩ . \norm{\Pi_{\eps,R}f}_2^2
\le C\E_\mu\inner{\Sigma\nabla f}{\nabla f}. ∥ Π ε , R f ∥ 2 2 ≤ C E μ ⟨ Σ∇ f , ∇ f ⟩ . Because H ≻ 0 H\succ0 H ≻ 0 and the support is connected, the kernel of A \Aop A consists of the constants. Thus f ⊥ ker A f\perp\ker\Aop f ⊥ ker A , and the spectral theorem gives Π ε , R f → f \Pi_{\eps,R}f\to f Π ε , R f → f in L 2 L^2 L 2 as R → ∞ R\to\infty R → ∞ and then ε ↓ 0 \eps\downarrow0 ε ↓ 0 .
For completeness, let H Σ 1 ( μ ) H^1_\Sigma(\mu) H Σ 1 ( μ ) be the closure of C \mathscr C C for the norm ∥ f ∥ 2 2 + E μ ⟨ Σ ∇ f , ∇ f ⟩ \norm f_2^2+\E_\mu\inner{\Sigma\nabla f}{\nabla f} ∥ f ∥ 2 2 + E μ ⟨ Σ∇ f , ∇ f ⟩ . Since Σ ≻ 0 \Sigma\succ0 Σ ≻ 0 is constant, this is the usual H 1 ( μ ) H^1(\mu) H 1 ( μ ) in the present regular setting. Approximate an arbitrary f ∈ H Σ 1 ( μ ) f\in H^1_\Sigma(\mu) f ∈ H Σ 1 ( μ ) by functions in C \mathscr C C and subtract their means. Variances and Σ \Sigma Σ -energies converge, so the inequality passes to the limit. Crucially, this argument does not claim that finite Σ \Sigma Σ -energy places f f f in the H H H -form domain when H H H is unbounded.
Only three properties of H H H enter: symmetry, positivity, and div μ H = − p \Div_\mu H=-p div μ H = − p . Neither log-concavity, nor the Monge–Ampère positivity (4.9) , nor Proposition D30.1 is used. Consequently the constant transfers with no loss, and the same reduction applies verbatim to any positive symmetric Stein kernel, not only the moment-map one.
4. The Hodge content: the affine channel and the solenoidal excess ¶ Let
A 1 = − div μ ( Σ ∇ ⋅ ) \Aop_1=-\Div_\mu(\Sigma\nabla\,\cdot\,) A 1 = − div μ ( Σ∇ ⋅ ) be the closed nonnegative self-adjoint operator associated with the covariance form
E Σ ( f , k ) = E μ ⟨ Σ ∇ f , ∇ k ⟩ , Dom ( E Σ ) = H Σ 1 ( μ ) , \calE_\Sigma(f,k)=\E_\mu\inner{\Sigma\nabla f}{\nabla k},
\qquad \Dom(\calE_\Sigma)=H^1_\Sigma(\mu), E Σ ( f , k ) = E μ ⟨ Σ∇ f , ∇ k ⟩ , Dom ( E Σ ) = H Σ 1 ( μ ) , and set L 0 2 ( μ ) = ( ker A 1 ) ⊥ L^2_0(\mu)=(\ker\Aop_1)^\perp L 0 2 ( μ ) = ( ker A 1 ) ⊥ . The support is connected and Σ ≻ 0 \Sigma\succ0 Σ ≻ 0 , so ker A 1 \ker\Aop_1 ker A 1 consists of the constants. Moreover C P a f f ( μ ) < ∞ \CPaff(\mu)<\infty C P aff ( μ ) < ∞ for each fixed full-dimensional log-concave probability measure (only a dimension-free bound is open). Consequently the restriction of A 1 \Aop_1 A 1 to L 0 2 ( μ ) L^2_0(\mu) L 0 2 ( μ ) has a bounded, everywhere-defined inverse
A 1 − 1 : L 0 2 ( μ ) ⟶ Dom ( A 1 ) ∩ L 0 2 ( μ ) . \Aop_1^{-1}:L^2_0(\mu)\longrightarrow
\Dom(\Aop_1)\cap L^2_0(\mu). A 1 − 1 : L 0 2 ( μ ) ⟶ Dom ( A 1 ) ∩ L 0 2 ( μ ) . Let g ∈ Dom ( A ) g\in\Dom(\Aop) g ∈ Dom ( A ) be such that u = H ∇ g ∈ L 2 ( μ ; Σ − 1 ) u=H\nabla g\in L^2(\mu;\Sigma^{-1}) u = H ∇ g ∈ L 2 ( μ ; Σ − 1 ) , and set
h = A g = − div μ u ∈ L 0 2 ( μ ) , ψ = A 1 − 1 h , w = u − Σ ∇ ψ . h=\Aop g=-\Div_\mu u\in L^2_0(\mu),\qquad
\psi=\Aop_1^{-1}h,\qquad
w=u-\Sigma\nabla\psi. h = A g = − div μ u ∈ L 0 2 ( μ ) , ψ = A 1 − 1 h , w = u − Σ∇ ψ . Then div μ w = 0 \Div_\mu w=0 div μ w = 0 ,
E μ ⟨ u , Σ − 1 u ⟩ = E μ ⟨ Σ ∇ ψ , ∇ ψ ⟩ + E μ ⟨ w , Σ − 1 w ⟩ , \E_\mu\inner{u}{\Sigma^{-1}u}
=\E_\mu\inner{\Sigma\nabla\psi}{\nabla\psi}+\E_\mu\inner{w}{\Sigma^{-1}w}, E μ ⟨ u , Σ − 1 u ⟩ = E μ ⟨ Σ∇ ψ , ∇ ψ ⟩ + E μ ⟨ w , Σ − 1 w ⟩ , and
sup 0 ≠ h ∈ L 0 2 ( μ ) E μ ⟨ Σ ∇ A 1 − 1 h , ∇ A 1 − 1 h ⟩ ∥ h ∥ 2 2 = C P a f f ( μ ) . \sup_{0\ne h\in L^2_0(\mu)}
\frac{\E_\mu\inner{\Sigma\nabla\Aop_1^{-1}h}
{\nabla\Aop_1^{-1}h}}
{\norm h_2^2}
=\CPaff(\mu). 0 = h ∈ L 0 2 ( μ ) sup ∥ h ∥ 2 2 E μ ⟨ Σ∇ A 1 − 1 h , ∇ A 1 − 1 h ⟩ = C P aff ( μ ) . Put H Σ = L 2 ( μ ; Σ − 1 ) \mathscr H_\Sigma=L^2(\mu;\Sigma^{-1}) H Σ = L 2 ( μ ; Σ − 1 ) and let
G Σ : H Σ 1 ( μ ) ⊂ L 2 ( μ ) ⟶ H Σ , G Σ f = Σ ∇ f . G_\Sigma:H^1_\Sigma(\mu)\subset L^2(\mu)\longrightarrow\mathscr H_\Sigma,
\qquad G_\Sigma f=\Sigma\nabla f. G Σ : H Σ 1 ( μ ) ⊂ L 2 ( μ ) ⟶ H Σ , G Σ f = Σ∇ f . This is a densely defined closed operator, its adjoint is the weak weighted divergence G Σ ∗ = − div μ G_\Sigma^*=-\Div_\mu G Σ ∗ = − div μ , and A 1 = G Σ ∗ G Σ \Aop_1=G_\Sigma^*G_\Sigma A 1 = G Σ ∗ G Σ . Here the assertion h = − div μ u ∈ L 2 h=-\Div_\mu u\in L^2 h = − div μ u ∈ L 2 means precisely that u ∈ Dom ( G Σ ∗ ) u\in\Dom(G_\Sigma^*) u ∈ Dom ( G Σ ∗ ) and G Σ ∗ u = h G_\Sigma^*u=h G Σ ∗ u = h : the usual integration-by-parts identity is first valid on the smooth core and extends to H Σ 1 ( μ ) H^1_\Sigma(\mu) H Σ 1 ( μ ) by closed-form density. Since ψ ∈ Dom ( A 1 ) \psi\in\Dom(\Aop_1) ψ ∈ Dom ( A 1 ) and A 1 ψ = h \Aop_1\psi=h A 1 ψ = h , we also have G Σ ψ ∈ Dom ( G Σ ∗ ) G_\Sigma\psi\in\Dom(G_\Sigma^*) G Σ ψ ∈ Dom ( G Σ ∗ ) and G Σ ∗ G Σ ψ = h G_\Sigma^*G_\Sigma\psi=h G Σ ∗ G Σ ψ = h . Therefore
w = u − G Σ ψ ∈ Dom ( G Σ ∗ ) , G Σ ∗ w = h − h = 0 , w=u-G_\Sigma\psi\in\Dom(G_\Sigma^*),
\qquad G_\Sigma^*w=h-h=0, w = u − G Σ ψ ∈ Dom ( G Σ ∗ ) , G Σ ∗ w = h − h = 0 , which is the weak statement div μ w = 0 \Div_\mu w=0 div μ w = 0 . The required integration by parts is now the adjoint identity at exactly these domains:
E μ ⟨ Σ ∇ ψ , Σ − 1 w ⟩ = ⟨ G Σ ψ , w ⟩ H Σ = ⟨ ψ , G Σ ∗ w ⟩ L 2 ( μ ) = 0. \E_\mu\inner{\Sigma\nabla\psi}{\Sigma^{-1}w}
=\inner{G_\Sigma\psi}{w}_{\mathscr H_\Sigma}
=\inner{\psi}{G_\Sigma^*w}_{L^2(\mu)}=0. E μ ⟨ Σ∇ ψ , Σ − 1 w ⟩ = ⟨ G Σ ψ , w ⟩ H Σ = ⟨ ψ , G Σ ∗ w ⟩ L 2 ( μ ) = 0. Thus G Σ ψ G_\Sigma\psi G Σ ψ and w w w are orthogonal in H Σ \mathscr H_\Sigma H Σ , and expanding u = G Σ ψ + w u=G_\Sigma\psi+w u = G Σ ψ + w gives the displayed Hodge identity. The same argument shows minimality: if v ∈ Dom ( G Σ ∗ ) v\in\Dom(G_\Sigma^*) v ∈ Dom ( G Σ ∗ ) and G Σ ∗ v = h G_\Sigma^*v=h G Σ ∗ v = h , then v − G Σ ψ ∈ ker G Σ ∗ v-G_\Sigma\psi\in\ker G_\Sigma^* v − G Σ ψ ∈ ker G Σ ∗ and hence
∥ v ∥ H Σ 2 = ∥ G Σ ψ ∥ H Σ 2 + ∥ v − G Σ ψ ∥ H Σ 2 . \norm v_{\mathscr H_\Sigma}^2
=\norm{G_\Sigma\psi}_{\mathscr H_\Sigma}^2
+\norm{v-G_\Sigma\psi}_{\mathscr H_\Sigma}^2. ∥ v ∥ H Σ 2 = ∥ G Σ ψ ∥ H Σ 2 + ∥ v − G Σ ψ ∥ H Σ 2 . Finally, for every h ∈ L 0 2 ( μ ) h\in L^2_0(\mu) h ∈ L 0 2 ( μ ) ,
E μ ⟨ Σ ∇ ψ , ∇ ψ ⟩ = ∥ G Σ ψ ∥ H Σ 2 = ⟨ A 1 ψ , ψ ⟩ L 2 ( μ ) = ⟨ h , A 1 − 1 h ⟩ L 2 ( μ ) . \E_\mu\inner{\Sigma\nabla\psi}{\nabla\psi}
=\norm{G_\Sigma\psi}_{\mathscr H_\Sigma}^2
=\inner{\Aop_1\psi}{\psi}_{L^2(\mu)}
=\inner{h}{\Aop_1^{-1}h}_{L^2(\mu)}. E μ ⟨ Σ∇ ψ , ∇ ψ ⟩ = ∥ G Σ ψ ∥ H Σ 2 = ⟨ A 1 ψ , ψ ⟩ L 2 ( μ ) = ⟨ h , A 1 − 1 h ⟩ L 2 ( μ ) . The spectral theorem for the positive self-adjoint restriction of A 1 \Aop_1 A 1 to L 0 2 ( μ ) L^2_0(\mu) L 0 2 ( μ ) therefore gives
sup 0 ≠ h ∈ L 0 2 ( μ ) ⟨ h , A 1 − 1 h ⟩ ∥ h ∥ 2 2 = ∥ A 1 − 1 ∥ = ( inf 0 ≠ f ∈ H Σ 1 ( μ ) f ⊥ ker A 1 E Σ ( f , f ) ∥ f ∥ 2 2 ) − 1 = C P a f f ( μ ) , \sup_{0\ne h\in L^2_0(\mu)}
\frac{\inner{h}{\Aop_1^{-1}h}}{\norm h_2^2}
=\norm{\Aop_1^{-1}}
=\left(
\inf_{\substack{0\ne f\in H^1_\Sigma(\mu)\\ f\perp\ker\Aop_1}}
\frac{\calE_\Sigma(f,f)}{\norm f_2^2}
\right)^{-1}
=\CPaff(\mu), 0 = h ∈ L 0 2 ( μ ) sup ∥ h ∥ 2 2 ⟨ h , A 1 − 1 h ⟩ = ∥ ∥ A 1 − 1 ∥ ∥ = ⎝ ⎛ 0 = f ∈ H Σ 1 ( μ ) f ⊥ k e r A 1 inf ∥ f ∥ 2 2 E Σ ( f , f ) ⎠ ⎞ − 1 = C P aff ( μ ) , where the last equality is exactly the variational definition (16.1) . This also verifies that no integration by parts has been applied outside the form/operator domains declared above.
Σ ∇ ψ \Sigma\nabla\psi Σ∇ ψ is the minimal-L 2 ( Σ − 1 ) L^2(\Sigma^{-1}) L 2 ( Σ − 1 ) field with divergence − h -h − h , and controlling it is precisely the affine Poincaré inequality. Hence C C M H ( μ ) ≥ C P a f f ( μ ) \CMH(\mu)\ge\CPaff(\mu) C CMH ( μ ) ≥ C P aff ( μ ) , and C M H ( C ) \mathrm{CMH}(C) CMH ( C ) implies C P a f f ( μ ) ≤ C \CPaff(\mu)\le C C P aff ( μ ) ≤ C . The only possible gap in the Hodge identity is the solenoidal excess E ⟨ w , Σ − 1 w ⟩ \E\inner{w}{\Sigma^{-1}w} E ⟨ w , Σ − 1 w ⟩ . In dimension one the no-flux convention forces w = 0 w=0 w = 0 , so C C M H = C P / Var \CMH=\CP/\Var C CMH = C P / Var exactly. In dimension at least two the divergence-free subspace is nontrivial, but the decomposition alone neither proves that w w w contributes at a CMH extremizer nor gives a measure for which C C M H > C P a f f \CMH>\CPaff C CMH > C P aff . Equivalence and strict nonimplication therefore remain open; in particular this corollary does not prove that C M H ( 4 ) \mathrm{CMH}(4) CMH ( 4 ) can fail while KLS holds.
5. Gate zero and the algebraic countermodel ¶ Testing (16.5) on g ( p ) = a ⋅ p g(p)=a\cdot p g ( p ) = a ⋅ p (so D 2 g = 0 D^2g=0 D 2 g = 0 , L μ g = − a ⋅ p L_\mu g=-a\cdot p L μ g = − a ⋅ p ) gives E ( L μ g ) 2 = a ⊤ Σ a \E(L_\mu g)^2=a^\top\Sigma a E ( L μ g ) 2 = a ⊤ Σ a and numerator a ⊤ E [ H Σ − 1 H ] a a^\top\E[H\Sigma^{-1}H]a a ⊤ E [ H Σ − 1 H ] a . Hence C M H ( 4 ) \mathrm{CMH}(4) CMH ( 4 ) implies gate zero , E [ H Σ − 1 H ] ⪯ 4 Σ \E[H\Sigma^{-1}H]\preceq4\Sigma E [ H Σ − 1 H ] ⪯ 4Σ , i.e. E H 2 ⪯ 4 I d \E H^2\preceq4\Id E H 2 ⪯ 4 Id in isotropic position (Conjecture 16.1 ).
For symmetric B , H B,H B , H : Tr ( B 2 H 2 ) = Tr ( B H B H ) + 1 2 ∥ [ B , H ] ∥ H S 2 \Tr(B^2H^2)=\Tr(BHBH)+\tfrac12\norm{[B,H]}_{\HS}^2 Tr ( B 2 H 2 ) = Tr ( B H B H ) + 2 1 ∥ [ B , H ] ∥ HS 2 .
[ B , H ] ⊤ = ( B H − H B ) ⊤ = H B − B H = − [ B , H ] [B,H]^\top=(BH-HB)^\top=HB-BH=-[B,H] [ B , H ] ⊤ = ( B H − H B ) ⊤ = H B − B H = − [ B , H ] , so [ B , H ] [B,H] [ B , H ] is antisymmetric and ∥ [ B , H ] ∥ H S 2 = Tr ( [ B , H ] [ B , H ] ⊤ ) = − Tr ( [ B , H ] 2 ) \norm{[B,H]}_{\HS}^2=\Tr([B,H][B,H]^\top)=-\Tr([B,H]^2) ∥ [ B , H ] ∥ HS 2 = Tr ([ B , H ] [ B , H ] ⊤ ) = − Tr ([ B , H ] 2 ) . Expanding [ B , H ] 2 = B H B H − B H 2 B − H B 2 H + H B H B [B,H]^2=BHBH-BH^2B-HB^2H+HBHB [ B , H ] 2 = B H B H − B H 2 B − H B 2 H + H B H B and taking traces gives Tr ( [ B , H ] 2 ) = 2 Tr ( B H B H ) − 2 Tr ( B 2 H 2 ) \Tr([B,H]^2)=2\Tr(BHBH)-2\Tr(B^2H^2) Tr ([ B , H ] 2 ) = 2 Tr ( B H B H ) − 2 Tr ( B 2 H 2 ) .
Let z z z be uniform on S m − 1 S^{m-1} S m − 1 , d = m / 2 m − 1 d=m/\sqrt{2m-1} d = m / 2 m − 1 , c = 1 − d / m c=1-d/m c = 1 − d / m , and H ( z ) = ( 1 d z ⊤ d z c I d m + d z z ⊤ ) H(z)=\left(\begin{smallmatrix}1&\sqrt d\,z^\top\\ \sqrt d\,z&c\Id_m+d\,zz^\top\end{smallmatrix}\right) H ( z ) = ( 1 d z d z ⊤ c Id m + d z z ⊤ ) .
Positivity. c > 0 c>0 c > 0 since d / m = 1 / 2 m − 1 < 1 d/m=1/\sqrt{2m-1}<1 d / m = 1/ 2 m − 1 < 1 , and the Schur complement of the ( 1 , 1 ) (1,1) ( 1 , 1 ) entry is c I d m + d z z ⊤ − d z z ⊤ = c I d m ≻ 0 c\Id_m+d\,zz^\top-d\,zz^\top=c\Id_m\succ0 c Id m + d z z ⊤ − d z z ⊤ = c Id m ≻ 0 ; hence H ⪰ 0 H\succeq0 H ⪰ 0 .
Normalization. E z = 0 \E z=0 E z = 0 kills the off-diagonal blocks and E z z ⊤ = I d m / m \E zz^\top=\Id_m/m E z z ⊤ = Id m / m gives E H = 1 ⊕ ( c + d / m ) I d m = I d m + 1 \E H=1\oplus(c+d/m)\Id_m=\Id_{m+1} E H = 1 ⊕ ( c + d / m ) Id m = Id m + 1 .
The quadratic form. With B = ( a r ⊤ r D ) B=\left(\begin{smallmatrix}a&r^\top\\r&D\end{smallmatrix}\right) B = ( a r r ⊤ D ) , expanding Tr ( B H B H ) \Tr(BHBH) Tr ( B H B H ) and using E z = 0 \E z=0 E z = 0 , E z z ⊤ = I d m / m \E zz^\top=\Id_m/m E z z ⊤ = Id m / m and E ( z ⊤ D z ) 2 = ( ( Tr D ) 2 + 2 Tr ( D 2 ) ) / ( m ( m + 2 ) ) \E(z^\top Dz)^2=\bigl((\Tr D)^2+2\Tr(D^2)\bigr)/(m(m+2)) E ( z ⊤ Dz ) 2 = ( ( Tr D ) 2 + 2 Tr ( D 2 ) ) / ( m ( m + 2 )) ,
E Tr ( B H B H ) = a 2 + 2 d m a Tr D + 2 ( c + 2 d m ) ∣ r ∣ 2 + ( c 2 + 2 c d m + 2 d 2 m ( m + 2 ) ) Tr ( D 2 ) + d 2 m ( m + 2 ) ( Tr D ) 2 . \begin{aligned}
\E\Tr(BHBH)&=a^2+\tfrac{2d}ma\Tr D+2\bigl(c+\tfrac{2d}m\bigr)\abs r^2\\
&\quad+\Bigl(c^2+\tfrac{2cd}m+\tfrac{2d^2}{m(m+2)}\Bigr)\Tr(D^2)
+\tfrac{d^2}{m(m+2)}(\Tr D)^2 .
\end{aligned} E Tr ( B H B H ) = a 2 + m 2 d a Tr D + 2 ( c + m 2 d ) ∣ r ∣ 2 + ( c 2 + m 2 c d + m ( m + 2 ) 2 d 2 ) Tr ( D 2 ) + m ( m + 2 ) d 2 ( Tr D ) 2 . Decompose D = t I d m + D 0 D=t\Id_m+D_0 D = t Id m + D 0 with Tr D 0 = 0 \Tr D_0=0 Tr D 0 = 0 . Then Tr D = m t \Tr D=mt Tr D = m t and Tr ( D 2 ) = m t 2 + Tr ( D 0 2 ) \Tr(D^2)=mt^2+\Tr(D_0^2) Tr ( D 2 ) = m t 2 + Tr ( D 0 2 ) , so the form splits into three O ( m ) O(m) O ( m ) -invariant sectors that do not interact: the vector sector ∣ r ∣ 2 \abs r^2 ∣ r ∣ 2 , the traceless sector Tr ( D 0 2 ) \Tr(D_0^2) Tr ( D 0 2 ) , and the two-dimensional scalar sector ( a , t ) (a,t) ( a , t ) .
Vector sector. Coefficient 2 ( c + 2 d / m ) = 2 ( 1 + d / m ) 2(c+2d/m)=2(1+d/m) 2 ( c + 2 d / m ) = 2 ( 1 + d / m ) , to be compared with 4 from 2 Tr ( B 2 ) 2\Tr(B^2) 2 Tr ( B 2 ) . Since d ≤ m d\le m d ≤ m (equivalently 2 m − 1 ≥ 1 \sqrt{2m-1}\ge1 2 m − 1 ≥ 1 ), it is at most 4.
Traceless sector. Coefficient c 2 + 2 c d / m + 2 d 2 / ( m ( m + 2 ) ) c^2+2cd/m+2d^2/(m(m+2)) c 2 + 2 c d / m + 2 d 2 / ( m ( m + 2 )) . Substituting c = 1 − d / m c=1-d/m c = 1 − d / m and d 2 = m 2 / ( 2 m − 1 ) d^2=m^2/(2m-1) d 2 = m 2 / ( 2 m − 1 ) gives 1 + m − 2 ( 2 m − 1 ) ( m + 2 ) 1+\frac{m-2}{(2m-1)(m+2)} 1 + ( 2 m − 1 ) ( m + 2 ) m − 2 , which is ≤ 2 \le2 ≤ 2 for all m ≥ 1 m\ge1 m ≥ 1 ; the comparison value is 2.
Scalar sector. With r = 0 r=0 r = 0 , D = t I d m D=t\Id_m D = t Id m , the above reduces to E Tr ( B H B H ) = a 2 + 2 d a t + t 2 ( m c 2 + 2 c d + d 2 ) \E\Tr(BHBH)=a^2+2dat+t^2\bigl(mc^2+2cd+d^2\bigr) E Tr ( B H B H ) = a 2 + 2 d a t + t 2 ( m c 2 + 2 c d + d 2 ) , and m c 2 + 2 c d + d 2 = m − 2 d + d 2 m + 2 d − 2 d 2 m + d 2 = m + d 2 − d 2 m mc^2+2cd+d^2=m-2d+\tfrac{d^2}m+2d-\tfrac{2d^2}m+d^2=m+d^2-\tfrac{d^2}m m c 2 + 2 c d + d 2 = m − 2 d + m d 2 + 2 d − m 2 d 2 + d 2 = m + d 2 − m d 2 . Hence the deficit is
2 ( a 2 + m t 2 ) − E Tr ( B H B H ) = a 2 − 2 d a t + [ m − d 2 ( 1 − 1 m ) ] t 2 . 2(a^2+mt^2)-\E\Tr(BHBH)=a^2-2dat+\Bigl[m-d^2\Bigl(1-\tfrac1m\Bigr)\Bigr]t^2 . 2 ( a 2 + m t 2 ) − E Tr ( B H B H ) = a 2 − 2 d a t + [ m − d 2 ( 1 − m 1 ) ] t 2 . The choice d 2 = m 2 / ( 2 m − 1 ) d^2=m^2/(2m-1) d 2 = m 2 / ( 2 m − 1 ) is exactly d 2 ( 2 − 1 m ) = m d^2(2-\tfrac1m)=m d 2 ( 2 − m 1 ) = m , i.e. m − d 2 ( 1 − 1 m ) = d 2 m-d^2(1-\tfrac1m)=d^2 m − d 2 ( 1 − m 1 ) = d 2 , so the deficit equals ( a − d t ) 2 ≥ 0 (a-dt)^2\ge0 ( a − d t ) 2 ≥ 0 — a perfect square, vanishing on the ray a = d t a=dt a = d t .
Combining the three sectors, E Tr ( B H B H ) ≤ 2 Tr ( B 2 ) \E\Tr(BHBH)\le2\Tr(B^2) E Tr ( B H B H ) ≤ 2 Tr ( B 2 ) for every symmetric B B B .
Failure of gate zero. ( H 2 ) 11 = 1 + d ∣ z ∣ 2 = 1 + d (H^2)_{11}=1+d\abs z^2=1+d ( H 2 ) 11 = 1 + d ∣ z ∣ 2 = 1 + d deterministically, so e 1 ⊤ E H 2 e 1 = 1 + d e_1^\top\E H^2e_1=1+d e 1 ⊤ E H 2 e 1 = 1 + d . Now 1 + d > 4 ⟺ d > 3 ⟺ m 2 > 9 ( 2 m − 1 ) ⟺ m 2 − 18 m + 9 > 0 1+d>4\iff d>3\iff m^2>9(2m-1)\iff m^2-18m+9>0 1 + d > 4 ⟺ d > 3 ⟺ m 2 > 9 ( 2 m − 1 ) ⟺ m 2 − 18 m + 9 > 0 , whose positive root is 9 + 6 2 ≈ 17.49 9+6\sqrt2\approx17.49 9 + 6 2 ≈ 17.49 ; hence the inequality holds exactly for integers m ≥ 18 m\ge18 m ≥ 18 .
The law above is not claimed to be a moment-map Hessian: no Monge–Ampère or Codazzi compatibility is imposed, and the proposition does not refute Conjecture 16.1 . What it proves is that positivity, E H = I d \E H=\Id E H = Id , and (4.15) do not imply gate zero by matrix algebra. By Lemma D30.2 the residual quantity any proof must control is E ∥ [ B , H ] ∥ H S 2 \E\norm{[B,H]}_{\HS}^2 E ∥ [ B , H ] ∥ HS 2 , and here it is maximal on the scalar ray a = d t a=dt a = d t where the Letwin deficit vanishes identically.
Obstructions respected. Route C carries no bounded_by edges: the six obstruction statements of the manuscript are scoped by their own statements to the fixed-cut Eldan program. The one with a method-level reach beyond it, rem:projection-ceiling, forbids proving quadratic-chaos thin shell from radial or projection information alone; nothing above uses projection tests — the endpoint reduction is a duality argument and the countermodel is exact finite-dimensional algebra. Remark 16.1 records that gate zero is an operator-to-trace upgrade of the same family as conj:trace-upgrade and conj:product-alignment; per the single-owner discipline of CLAUDE.md, no claim of equivalence with those nodes is made here.
Numerical status. The cmh-gate-zero numerics target computes λ max ( Σ − 1 / 2 E [ H Σ − 1 H ] Σ − 1 / 2 ) \lmax(\Sigma^{-1/2}\E[H\Sigma^{-1}H]\Sigma^{-1/2}) λ m a x ( Σ − 1/2 E [ H Σ − 1 H ] Σ − 1/2 ) in closed form on one-dimensional laws, products, and from exact moment matrices on the Dirichlet family, and regression-tests the sector identities of Proposition D30.3 . Only an exact rational certificate may refute Conjecture 16.1 ; floating eigenvalues and Galerkin optima are directional. The current battery lies inside already-proved classes and contributes nothing to the analytic theorems above.
Conditional template beyond the regular class. Let μ q \mu_q μ q be the regular approximants from §Sources , chosen so that μ q → μ \mu_q\to\mu μ q → μ with second moments and therefore Σ q → Σ \Sigma_q\to\Sigma Σ q → Σ . If sup q C C M H ( μ q ) ≤ C \sup_q\CMH(\mu_q)\le C sup q C CMH ( μ q ) ≤ C , Theorem D30.1 applied to a fixed f ∈ C c ∞ f\in C_c^\infty f ∈ C c ∞ gives
Var μ q f ≤ C ∫ ⟨ Σ q ∇ f , ∇ f ⟩ d μ q . \Var_{\mu_q}f\le C\int\inner{\Sigma_q\nabla f}{\nabla f}\,d\mu_q. Var μ q f ≤ C ∫ ⟨ Σ q ∇ f , ∇ f ⟩ d μ q . The two sides converge because f f f and ∇ f \nabla f ∇ f are bounded and continuous and the second moments converge. Subject to a limiting H Σ 1 ( μ ) H^1_\Sigma(\mu) H Σ 1 ( μ ) core-density theorem, the endpoint argument then extends the inequality to the full Sobolev domain. No continuity of C C M H \CMH C CMH is used or claimed. A complete proof must still construct approximants with the asserted moment and affine-support behavior and justify this density passage; those obligations are precisely Proposition 15.1 .