Write p = C P ( μ ) < ∞ p=C_P(\mu)<\infty p = C P ( μ ) < ∞ , K = D 2 V K=D^2V K = D 2 V , and w = Z − 1 e − V w=Z^{-1}e^{-V} w = Z − 1 e − V .
All tensor norms sum over ordered indices; exterior norms sum over increasing
indices. Distributional derivatives are meaningful because the weight is
positive and smooth and weighted L 2 L^2 L 2 convergence implies local distributional
convergence.
Finite-energy primitives. First, if h ∈ W l o c 1 , 2 h\in W^{1,2}_{\rm loc} h ∈ W loc 1 , 2 and
∇ h ∈ L 2 ( μ ) \nabla h\in L^2(\mu) ∇ h ∈ L 2 ( μ ) , then h ∈ L 2 ( μ ) h\in L^2(\mu) h ∈ L 2 ( μ ) and
Var μ h ≤ p ∥ ∇ h ∥ 2 2 \operatorname{Var}_\mu h\le p\|\nabla h\|_2^2 Var μ h ≤ p ∥∇ h ∥ 2 2 . Here is the extension
argument, which avoids assuming the desired integrability. The scalar inequality
extends to compactly supported Sobolev functions by mollification on compact
sets. For bounded locally Sobolev h h h , multiply by a smooth cutoff χ R \chi_R χ R
with ∣ ∇ χ R ∣ ≤ C / R |\nabla\chi_R|\le C/R ∣∇ χ R ∣ ≤ C / R ; both function and gradient converge in weighted
L 2 L^2 L 2 . Thus the inequality holds for bounded finite-energy functions. Apply it
to h N = max ( − N , min ( h , N ) ) h_N=\max(-N,\min(h,N)) h N = max ( − N , min ( h , N )) . Their variances are uniformly bounded by
E = p ∥ ∇ h ∥ 2 2 E=p\|\nabla h\|_2^2 E = p ∥∇ h ∥ 2 2 . Choose M M M such that
A = { ∣ h ∣ ≤ M } A=\{|h|\le M\} A = { ∣ h ∣ ≤ M } has positive measure. For N ≥ M N\ge M N ≥ M and
m N = E h N m_N=\mathbb Eh_N m N = E h N ,
μ ( A ) ( ∣ m N ∣ − M ) + 2 ≤ Var ( h N ) ≤ E . \mu(A)(|m_N|-M)_+^2\le\operatorname{Var}(h_N)\le E. μ ( A ) ( ∣ m N ∣ − M ) + 2 ≤ Var ( h N ) ≤ E . The means and hence ∥ h N ∥ 2 \|h_N\|_2 ∥ h N ∥ 2 are bounded. Fatou gives h ∈ L 2 h\in L^2 h ∈ L 2 ;
then h N → h h_N\to h h N → h in L 2 L^2 L 2 proves the asserted variance inequality.
A locally square-integrable curl-free vector field has a global locally
W 1 , 2 W^{1,2} W 1 , 2 primitive on R n \mathbb R^n R n . Explicitly, mollify it, integrate the
resulting smooth field along the segment from zero to x x x , and subtract its
Lebesgue mean on the unit ball. On each larger ball the gradient converges in
L 2 L^2 L 2 ; the ordinary Poincaré inequality together with the fixed mean controls
the additive constant. These primitives converge locally in W 1 , 2 W^{1,2} W 1 , 2 .
For F ∈ C r + 1 F\in C_{r+1} F ∈ C r + 1 do this for each vector ( F i I ) i (F_{iI})_i ( F i I ) i and center the
primitive using the finite-energy result. Denote it by U I U_I U I . Permuting I I I
preserves its gradient, so uniqueness of a centered primitive makes U U U
symmetric. Moreover ∂ i U j I = F i j I = ∂ j U i I \partial_iU_{jI}=F_{ijI}=\partial_jU_{iI} ∂ i U j I = F ij I = ∂ j U i I , so U U U is
compatible. Summing the scalar inequalities yields
∇ U = F , E U = 0 , ∥ U ∥ 2 2 ≤ p ∥ F ∥ 2 2 . \nabla U=F,\qquad \mathbb EU=0,\qquad \|U\|_2^2\le p\|F\|_2^2. ∇ U = F , E U = 0 , ∥ U ∥ 2 2 ≤ p ∥ F ∥ 2 2 . Uniqueness follows from vanishing gradient and centering.
Potential cores. Repeated primitive construction writes every F ∈ C r F\in C_r F ∈ C r
as F = ∇ r ϕ F=\nabla^r\phi F = ∇ r ϕ with ϕ ∈ W r , 2 ( μ ) \phi\in W^{r,2}(\mu) ϕ ∈ W r , 2 ( μ ) ; if additionally
F ∈ W 1 , 2 F\in W^{1,2} F ∈ W 1 , 2 , then ϕ ∈ W r + 1 , 2 \phi\in W^{r+1,2} ϕ ∈ W r + 1 , 2 . Let χ R \chi_R χ R be compactly
supported, equal to one on B R B_R B R , with
∣ ∇ j χ R ∣ ≤ C j R − j |\nabla^j\chi_R|\le C_jR^{-j} ∣ ∇ j χ R ∣ ≤ C j R − j . The product rule gives
χ R ϕ → ϕ \chi_R\phi\to\phi χ R ϕ → ϕ in every indicated weighted Sobolev norm: the terms
with cutoff derivatives are bounded by C j R − j C_jR^{-j} C j R − j times lower derivative
norms and the term without cutoff derivatives converges by dominated
convergence. Mollification at fixed compact support is valid since w , w − 1 w,w^{-1} w , w − 1
are bounded there. A diagonal sequence proves that K r \mathcal K_r K r is dense
in C r C_r C r and is a graph core for its maximal ordinary derivative. Subtracting
expectations proves the centered versions in G r G_r G r . These assertions also hold
at r = 0 r=0 r = 0 by the direct cutoff argument. Closedness of the distributional
derivative now proves that D r D_r D r is closed and densely defined. The primitive
construction makes it bijective with the asserted bounded inverse.
One missing weak derivative. We need the following fact for the adjoint
core. Suppose q ≥ 1 q\ge1 q ≥ 1 , ϕ ∈ W q − 1 , 2 ( μ ) \phi\in W^{q-1,2}(\mu) ϕ ∈ W q − 1 , 2 ( μ ) and
G ∈ L 2 ( μ ; ( R n ) ⊗ q ) G\in L^2(\mu;(\mathbb R^n)^{\otimes q}) G ∈ L 2 ( μ ; ( R n ) ⊗ q ) satisfy
∫ ⟨ ∇ q ϕ , ∇ q ψ ⟩ d μ = ∫ ⟨ G , ∇ q ψ ⟩ d μ ( ψ ∈ C c ∞ ) , (1) \int\langle\nabla^q\phi,\nabla^q\psi\rangle\,d\mu
=\int\langle G,\nabla^q\psi\rangle\,d\mu
\quad(\psi\in C_c^\infty), \tag{1} ∫ ⟨ ∇ q ϕ , ∇ q ψ ⟩ d μ = ∫ ⟨ G , ∇ q ψ ⟩ d μ ( ψ ∈ C c ∞ ) , ( 1 ) where the left side is a distributional pairing. Then
ϕ ∈ W q , 2 ( μ ) \phi\in W^{q,2}(\mu) ϕ ∈ W q , 2 ( μ ) . Indeed the distributional equation is
∑ I ∂ I ( w ∂ I ϕ ) = ∑ I ∂ I ( w G I ) \sum_I\partial_I(w\partial_I\phi)=\sum_I\partial_I(wG_I) ∑ I ∂ I ( w ∂ I ϕ ) = ∑ I ∂ I ( w G I ) .
After expanding derivatives of w w w , the leading part is w Δ q ϕ w\Delta^q\phi w Δ q ϕ ;
the other terms have order at most 2 q − 1 2q-1 2 q − 1 on ϕ \phi ϕ . Thus
Δ q ϕ ∈ H l o c − q \Delta^q\phi\in H^{-q}_{\rm loc} Δ q ϕ ∈ H loc − q . For a compact smooth ζ \zeta ζ ,
Δ q ( ζ ϕ ) ∈ H − q \Delta^q(\zeta\phi)\in H^{-q} Δ q ( ζϕ ) ∈ H − q because the commutator has order
2 q − 1 2q-1 2 q − 1 , and ζ ϕ ∈ H q − 1 \zeta\phi\in H^{q-1} ζϕ ∈ H q − 1 . In Fourier variables the high
frequencies satisfy
∣ ξ ∣ 4 q ( 1 + ∣ ξ ∣ 2 ) q ≍ ( 1 + ∣ ξ ∣ 2 ) q ( ∣ ξ ∣ ≥ 1 ) , \frac{|\xi|^{4q}}{(1+|\xi|^2)^q}\asymp(1+|\xi|^2)^q
\quad(|\xi|\ge1), ( 1 + ∣ ξ ∣ 2 ) q ∣ ξ ∣ 4 q ≍ ( 1 + ∣ ξ ∣ 2 ) q ( ∣ ξ ∣ ≥ 1 ) , while the H q − 1 H^{q-1} H q − 1 norm controls the low frequencies. Hence
ϕ ∈ H l o c q \phi\in H^q_{\rm loc} ϕ ∈ H loc q .
Choose 0 ≤ η ≤ 1 0\le\eta\le1 0 ≤ η ≤ 1 compactly supported, equal to one near zero, and
η R ( x ) = η ( x / R ) \eta_R(x)=\eta(x/R) η R ( x ) = η ( x / R ) . Local regularity permits the Sobolev test
ψ = η R 2 q ϕ \psi=\eta_R^{2q}\phi ψ = η R 2 q ϕ in (1). The product rule gives
∇ q ( η R 2 q ϕ ) = η R 2 q ∇ q ϕ + R R , ∣ R R ∣ ≤ C q η R q ∑ j = 1 q R − j ∣ ∇ q − j ϕ ∣ . \nabla^q(\eta_R^{2q}\phi)=\eta_R^{2q}\nabla^q\phi+R_R,
\qquad |R_R|\le C_q\eta_R^q\sum_{j=1}^qR^{-j}|\nabla^{q-j}\phi|. ∇ q ( η R 2 q ϕ ) = η R 2 q ∇ q ϕ + R R , ∣ R R ∣ ≤ C q η R q j = 1 ∑ q R − j ∣ ∇ q − j ϕ ∣. For the power of η R \eta_R η R , regard η R 2 q \eta_R^{2q} η R 2 q as a product of 2 q 2q 2 q
factors: at least q q q remain undifferentiated in every remainder term.
Set A R = ∥ η R q ∇ q ϕ ∥ 2 A_R=\|\eta_R^q\nabla^q\phi\|_2 A R = ∥ η R q ∇ q ϕ ∥ 2 and
b R = C q ∑ j = 1 q R − j ∥ ∇ q − j ϕ ∥ 2 b_R=C_q\sum_{j=1}^qR^{-j}\|\nabla^{q-j}\phi\|_2 b R = C q ∑ j = 1 q R − j ∥ ∇ q − j ϕ ∥ 2 .
Both ∥ R R ∥ 2 \|R_R\|_2 ∥ R R ∥ 2 and ∥ R R / η R q ∥ 2 \|R_R/\eta_R^q\|_2 ∥ R R / η R q ∥ 2 are at most b R b_R b R ,
with zero quotient where η R = 0 \eta_R=0 η R = 0 . Equation (1) yields
A R 2 ≤ A R ( ∥ G ∥ 2 + b R ) + ∥ G ∥ 2 b R , A R ≤ ∥ G ∥ 2 + 2 b R . A_R^2\le A_R(\|G\|_2+b_R)+\|G\|_2b_R,
\qquad A_R\le\|G\|_2+2b_R. A R 2 ≤ A R ( ∥ G ∥ 2 + b R ) + ∥ G ∥ 2 b R , A R ≤ ∥ G ∥ 2 + 2 b R . Since b R → 0 b_R\to0 b R → 0 , Fatou supplies the missing global derivative.
The adjoint graph core. On K r + 1 \mathcal K_{r+1} K r + 1 define
S r F = P G r div V F S_rF=P_{G_r}\operatorname{div}_VF S r F = P G r div V F , where
( div V F ) I = ∑ j ( − ∂ j + V j ) F I j (\operatorname{div}_VF)_I=\sum_j(-\partial_j+V_j)F_{Ij} ( div V F ) I = ∑ j ( − ∂ j + V j ) F I j .
Integration by parts gives S r ⊂ D r ∗ S_r\subset D_r^* S r ⊂ D r ∗ , hence closability; its domain
is dense by the potential-core argument. We show S r ∗ = D r S_r^*=D_r S r ∗ = D r .
The forward inclusion D r ⊂ S r ∗ D_r\subset S_r^* D r ⊂ S r ∗ is integration by parts. If
u ∈ Dom ( S r ∗ ) u\in\operatorname{Dom}(S_r^*) u ∈ Dom ( S r ∗ ) with g = S r ∗ u g=S_r^*u g = S r ∗ u , write
u = ∇ r ϕ u=\nabla^r\phi u = ∇ r ϕ with ϕ ∈ W r , 2 \phi\in W^{r,2} ϕ ∈ W r , 2 (and ϕ = u \phi=u ϕ = u if r = 0 r=0 r = 0 ).
The adjoint equation tested against ∇ r + 1 ψ \nabla^{r+1}\psi ∇ r + 1 ψ is exactly (1)
with q = r + 1 q=r+1 q = r + 1 and G = g G=g G = g . Thus ∇ u ∈ L 2 \nabla u\in L^2 ∇ u ∈ L 2 and u ∈ Dom ( D r ) u\in\operatorname{Dom}(D_r) u ∈ Dom ( D r ) .
Density of K r + 1 \mathcal K_{r+1} K r + 1 identifies D r u = g D_ru=g D r u = g . Taking adjoints proves
S ‾ r = D r ∗ \overline S_r=D_r^* S r = D r ∗ . This proves graph approximation of the adjoint,
not merely norm approximation of its domain.
Weighted divergence and projection loss. It remains to prove the estimate
on this core. Fix m ≥ 0 m\ge0 m ≥ 0 and F = ∇ m + 1 ψ F=\nabla^{m+1}\psi F = ∇ m + 1 ψ with compact smooth
ψ \psi ψ , and put Y = div V F Y=\operatorname{div}_VF Y = div V F . Integration by parts gives
E Y = 0 \mathbb EY=0 E Y = 0 and
D m ∗ F = P G m Y = P C m Y D_m^*F=P_{G_m}Y=P_{C_m}Y D m ∗ F = P G m Y = P C m Y . Since [ ∂ i , ∂ j ∗ ] = V i j [\partial_i,\partial_j^*]=V_{ij} [ ∂ i , ∂ j ∗ ] = V ij
and ∇ F \nabla F ∇ F is fully symmetric, two integrations by parts give
∥ P C m Y ∥ 2 2 = ∥ ∇ F ∥ 2 2 + B K ( F ) − ∥ ( I − P C m ) Y ∥ 2 2 , B K ( F ) = E ∑ I , i , j V i j F I i F I j . (2) \|P_{C_m}Y\|_2^2=\|\nabla F\|_2^2+B_K(F)-\|(I-P_{C_m})Y\|_2^2,
\quad B_K(F)=\mathbb E\sum_{I,i,j}V_{ij}F_{Ii}F_{Ij}. \tag{2} ∥ P C m Y ∥ 2 2 = ∥∇ F ∥ 2 2 + B K ( F ) − ∥ ( I − P C m ) Y ∥ 2 2 , B K ( F ) = E I , i , j ∑ V ij F I i F I j . ( 2 ) If m = 0 m=0 m = 0 , C 0 = L 2 C_0=L^2 C 0 = L 2 and there is no projection loss; B K ( F ) ≥ a ∥ F ∥ 2 2 B_K(F)\ge a\|F\|_2^2 B K ( F ) ≥ a ∥ F ∥ 2 2
finishes this case. Henceforth m ≥ 1 m\ge1 m ≥ 1 . Differentiation and compatibility
cancel all derivatives of F F F in the curl of Y Y Y :
∂ k Y l I − ∂ l Y k I = ∑ j ( V k j F l I j − V l j F k I j ) , ∣ I ∣ = m − 1. (3) \partial_kY_{lI}-\partial_lY_{kI}
=\sum_j(V_{kj}F_{lIj}-V_{lj}F_{kIj}),\qquad |I|=m-1. \tag{3} ∂ k Y l I − ∂ l Y k I = j ∑ ( V kj F l I j − V l j F k I j ) , ∣ I ∣ = m − 1. ( 3 ) A constrained complex with all domains specified. On normalized symmetric
basis vectors e α e_\alpha e α define
a i e α = α i e α − e i a_ie_\alpha=\sqrt{\alpha_i}e_{\alpha-e_i} a i e α = α i e α − e i and
a i ∗ e α = α i + 1 e α + e i a_i^*e_\alpha=\sqrt{\alpha_i+1}e_{\alpha+e_i} a i ∗ e α = α i + 1 e α + e i .
Contraction in one slot of a rank-q q q tensor is a i / q a_i/\sqrt q a i / q .
Let ε i \varepsilon_i ε i be exterior multiplication and ι i \iota_i ι i its adjoint.
They satisfy [ a i , a j ∗ ] = δ i j [a_i,a_j^*]=\delta_{ij} [ a i , a j ∗ ] = δ ij and
ι j ε i + ε i ι j = δ i j \iota_j\varepsilon_i+\varepsilon_i\iota_j=\delta_{ij} ι j ε i + ε i ι j = δ ij .
Define b = ∑ i a i ε i b=\sum_i a_i\varepsilon_i b = ∑ i a i ε i on the entire symmetric/exterior algebra.
It obeys b 2 = 0 b^2=0 b 2 = 0 and, at bidegree ( q , p ) (q,p) ( q , p ) ,
b b ∗ + b ∗ b = ( q + p ) I . bb^*+b^*b=(q+p)I. b b ∗ + b ∗ b = ( q + p ) I . Indeed the mixed terms cancel after commuting the two sorts of operators;
the terms remaining are the symmetric and exterior number operators.
Fix q = m − 1 q=m-1 q = m − 1 , set E p = ker b ⊂ Sym m − 1 ⊗ Λ p \mathscr E_p=\ker b\subset\operatorname{Sym}^{m-1}\otimes\Lambda^p E p = ker b ⊂ Sym m − 1 ⊗ Λ p
for p ≥ 1 p\ge1 p ≥ 1 , and let P p = b b ∗ / ( m + p − 1 ) P_p=bb^*/(m+p-1) P p = b b ∗ / ( m + p − 1 ) be its orthogonal projection.
The map I m T = b T / m I_mT=bT/\sqrt m I m T = b T / m is an isometry of E m E_m E m onto E 1 \mathscr E_1 E 1 :
b ∗ b = m I b^*b=mI b ∗ b = m I on E m E_m E m , and b b ∗ = m I bb^*=mI b b ∗ = m I on E 1 \mathscr E_1 E 1 proves surjectivity.
Let d = ∑ i ε i ∂ i d=\sum_i\varepsilon_i\partial_i d = ∑ i ε i ∂ i and give
d p : L 2 ( μ ; E p ) → L 2 ( μ ; E p + 1 ) d_p:L^2(\mu;\mathscr E_p)\to L^2(\mu;\mathscr E_{p+1}) d p : L 2 ( μ ; E p ) → L 2 ( μ ; E p + 1 ) its maximal
distributional domain. The identity b d + d b = 0 bd+db=0 b d + d b = 0 preserves the constraint;
d p + 1 d p = 0 d_{p+1}d_p=0 d p + 1 d p = 0 including its domain inclusion. These operators are closed
and densely defined. Their adjoints are the maximal expressions
d p ∗ = P p d ∗ d_p^*=P_pd^* d p ∗ = P p d ∗ , d ∗ = ∑ i ι i ( − ∂ i + V i ) d^*=\sum_i\iota_i(-\partial_i+V_i) d ∗ = ∑ i ι i ( − ∂ i + V i ) .
Here are the domain details. Cutoff commutators with these first-order
expressions are bounded pointwise by C ∣ ∇ χ R ∣ ∣ ω ∣ C|\nabla\chi_R||\omega| C ∣∇ χ R ∣∣ ω ∣ and converge
to zero in L 2 L^2 L 2 . On fixed compact supports convolution commutes with all
constant derivative coefficients and fiber projections. The only coefficient
commutator is
V i ( x ) ( ω ∗ ρ ϵ ) ( x ) − ( V i ω ) ∗ ρ ϵ ( x ) = ∫ ρ ϵ ( y ) [ V i ( x ) − V i ( x − y ) ] ω ( x − y ) d y . V_i(x)(\omega*\rho_\epsilon)(x)-(V_i\omega)*\rho_\epsilon(x)
=\int\rho_\epsilon(y)[V_i(x)-V_i(x-y)]\omega(x-y)\,dy. V i ( x ) ( ω ∗ ρ ϵ ) ( x ) − ( V i ω ) ∗ ρ ϵ ( x ) = ∫ ρ ϵ ( y ) [ V i ( x ) − V i ( x − y )] ω ( x − y ) d y . Its local L 2 L^2 L 2 norm is at most C ϵ ∥ ω ∥ L 2 ( d x ) C\epsilon\|\omega\|_{L^2(dx)} C ϵ ∥ ω ∥ L 2 ( d x ) by
local Lipschitz continuity and Young’s inequality. Equivalence of weights on
compact sets proves convergence in weighted L 2 L^2 L 2 . Consequently compact
smooth sections are simultaneous graph cores for each needed maximal
expression, in particular d 2 d_2 d 2 and d 1 ∗ d_1^* d 1 ∗ . Testing against compact sections
first characterizes the Hilbert adjoint distributionally; this graph
approximation extends integration by parts to the maximal domains and proves
the converse inclusion. Finally I m C m = ker d 1 I_mC_m=\ker d_1 I m C m = ker d 1 , since these kernel
equations are precisely the compatibility equations.
The Laplacian curvature estimate. On L 2 ( μ ; E 2 ) L^2(\mu;\mathscr E_2) L 2 ( μ ; E 2 ) let
L \mathcal L L represent the closed densely defined form
ℓ ( ω ) = ∥ d 2 ω ∥ 2 2 + ∥ d 1 ∗ ω ∥ 2 2 , \ell(\omega)=\|d_2\omega\|_2^2+\|d_1^*\omega\|_2^2, ℓ ( ω ) = ∥ d 2 ω ∥ 2 2 + ∥ d 1 ∗ ω ∥ 2 2 , with form domain Dom ( d 2 ) ∩ Dom ( d 1 ∗ ) \operatorname{Dom}(d_2)\cap\operatorname{Dom}(d_1^*) Dom ( d 2 ) ∩ Dom ( d 1 ∗ ) .
Initially take compact smooth ω \omega ω . Set
K f e r = ∑ i , j V i j ε i ι j , K b o s = ∑ i , j V i j a j ∗ a i , c = ∑ i a i ∂ i ∗ . K_{\rm fer}=\sum_{i,j}V_{ij}\varepsilon_i\iota_j,
\quad K_{\rm bos}=\sum_{i,j}V_{ij}a_j^*a_i,
\quad c=\sum_i a_i\partial_i^*. K fer = i , j ∑ V ij ε i ι j , K bos = i , j ∑ V ij a j ∗ a i , c = i ∑ a i ∂ i ∗ . The ordinary weighted Weitzenböck identity, obtained by expanding d d ∗ + d ∗ d dd^*+d^*d d d ∗ + d ∗ d ,
is
∥ d ω ∥ 2 2 + ∥ d ∗ ω ∥ 2 2 = ∥ ∇ ω ∥ 2 2 + E ⟨ ω , K f e r ω ⟩ \|d\omega\|_2^2+\|d^*\omega\|_2^2
=\|\nabla\omega\|_2^2+\mathbb E\langle\omega,K_{\rm fer}\omega\rangle ∥ d ω ∥ 2 2 + ∥ d ∗ ω ∥ 2 2 = ∥∇ ω ∥ 2 2 + E ⟨ ω , K fer ω ⟩ .
Since I − P 1 = b ∗ b / m I-P_1=b^*b/m I − P 1 = b ∗ b / m and b d ∗ + d ∗ b = c bd^*+d^*b=c b d ∗ + d ∗ b = c , one obtains
ℓ ( ω ) = ∥ ∇ ω ∥ 2 2 + E ⟨ ω , K f e r ω ⟩ − m − 1 ∥ c ω ∥ 2 2 . \ell(\omega)=\|\nabla\omega\|_2^2+
\mathbb E\langle\omega,K_{\rm fer}\omega\rangle-m^{-1}\|c\omega\|_2^2. ℓ ( ω ) = ∥∇ ω ∥ 2 2 + E ⟨ ω , K fer ω ⟩ − m − 1 ∥ c ω ∥ 2 2 . Moreover [ c , c ∗ ] = H − K b o s [c,c^*]=H-K_{\rm bos} [ c , c ∗ ] = H − K bos , where
H = ∑ i ∂ i ∗ ∂ i H=\sum_i\partial_i^*\partial_i H = ∑ i ∂ i ∗ ∂ i acts componentwise. The row map
( a i ∗ ) i (a_i^*)_i ( a i ∗ ) i from copies of degree m − 1 m-1 m − 1 to degree m m m has norm m \sqrt m m ,
as its product with its adjoint is ∑ i a i ∗ a i = m I \sum_i a_i^*a_i=mI ∑ i a i ∗ a i = m I . Therefore
∥ c ω ∥ 2 2 = ∥ c ∗ ω ∥ 2 2 − ∥ ∇ ω ∥ 2 2 + E ⟨ ω , K b o s ω ⟩ ≤ ( m − 1 ) ∥ ∇ ω ∥ 2 2 + E ⟨ ω , K b o s ω ⟩ . \|c\omega\|_2^2=\|c^*\omega\|_2^2-\|\nabla\omega\|_2^2
+\mathbb E\langle\omega,K_{\rm bos}\omega\rangle
\le(m-1)\|\nabla\omega\|_2^2+
\mathbb E\langle\omega,K_{\rm bos}\omega\rangle. ∥ c ω ∥ 2 2 = ∥ c ∗ ω ∥ 2 2 − ∥∇ ω ∥ 2 2 + E ⟨ ω , K bos ω ⟩ ≤ ( m − 1 ) ∥∇ ω ∥ 2 2 + E ⟨ ω , K bos ω ⟩ . It follows that
ℓ ( ω ) ≥ m − 1 ∥ ∇ ω ∥ 2 2 + E ⟨ ω , Q m ( K ) ω ⟩ , Q m ( K ) = P 2 ( K f e r − m − 1 K b o s ) P 2 . (4) \ell(\omega)\ge m^{-1}\|\nabla\omega\|_2^2+
\mathbb E\langle\omega,Q_m(K)\omega\rangle,
\qquad Q_m(K)=P_2(K_{\rm fer}-m^{-1}K_{\rm bos})P_2. \tag{4} ℓ ( ω ) ≥ m − 1 ∥∇ ω ∥ 2 2 + E ⟨ ω , Q m ( K ) ω ⟩ , Q m ( K ) = P 2 ( K fer − m − 1 K bos ) P 2 . ( 4 ) Exact curvature blocks. Diagonalize K K K pointwise, with eigenvalues
κ i ≥ a \kappa_i\ge a κ i ≥ a . All calculations here are orthogonally invariant and use
no derivatives of this diagonalizing basis. Put N = m + 1 N=m+1 N = m + 1 . The combined
multiplicity α \alpha α of symmetric and exterior indices has ∣ α ∣ = N |\alpha|=N ∣ α ∣ = N .
In each block restrict coordinates to S α = { i : α i > 0 } S_\alpha=\{i:\alpha_i>0\} S α = { i : α i > 0 } ,
write r i = α i r_i=\sqrt{\alpha_i} r i = α i and S = ∑ i α i κ i S=\sum_i\alpha_i\kappa_i S = ∑ i α i κ i .
Then ∣ r ∣ 2 = N |r|^2=N ∣ r ∣ 2 = N , and b b b is exterior multiplication by r r r . Thus the constrained
two-forms are exactly ω = r ∧ v \omega=r\wedge v ω = r ∧ v , v ⊥ r v\perp r v ⊥ r , with
∥ ω ∥ 2 = N ∣ v ∣ 2 \|\omega\|^2=N|v|^2 ∥ ω ∥ 2 = N ∣ v ∣ 2 . This also follows from
ι r ( r ∧ ω ) + r ∧ ι r ω = N ω \iota_r(r\wedge\omega)+r\wedge\iota_r\omega=N\omega ι r ( r ∧ ω ) + r ∧ ι r ω = N ω .
If the coordinate support has one element, the two-form space is zero;
all formulas below have their zero-space meanings.
On the exterior pair i j ij ij , K f e r − m − 1 K b o s K_{\rm fer}-m^{-1}K_{\rm bos} K fer − m − 1 K bos has coefficient
[ N ( κ i + κ j ) − S ] / m [N(\kappa_i+\kappa_j)-S]/m [ N ( κ i + κ j ) − S ] / m . Expanding squares, and using r ⋅ v = 0 r\cdot v=0 r ⋅ v = 0 ,
gives
∑ i < j ( κ i + κ j ) ( r i v j − r j v i ) 2 = S ∣ v ∣ 2 + N ⟨ v , K v ⟩ . \sum_{i<j}(\kappa_i+\kappa_j)(r_iv_j-r_jv_i)^2
=S|v|^2+N\langle v,Kv\rangle. i < j ∑ ( κ i + κ j ) ( r i v j − r j v i ) 2 = S ∣ v ∣ 2 + N ⟨ v , K v ⟩ . Consequently
⟨ r ∧ v , Q m ( K ) ( r ∧ v ) ⟩ = N 2 m ⟨ v , K v ⟩ . (5) \langle r\wedge v,Q_m(K)(r\wedge v)\rangle
=\frac{N^2}{m}\langle v,Kv\rangle. \tag{5} ⟨ r ∧ v , Q m ( K ) ( r ∧ v )⟩ = m N 2 ⟨ v , K v ⟩ . ( 5 ) In particular Q m ( K ) ⪰ ( N / m ) a I Q_m(K)\succeq(N/m)aI Q m ( K ) ⪰ ( N / m ) a I . If P P P projects onto r ⊥ r^\perp r ⊥ ,
the isometry U v = ( r / N ) ∧ v Uv=(r/\sqrt N)\wedge v Uv = ( r / N ) ∧ v satisfies
U ∗ Q m ( K ) U = ( N / m ) ( P K P ) ∣ r ⊥ U^*Q_m(K)U=(N/m)(PKP)|_{r^\perp} U ∗ Q m ( K ) U = ( N / m ) ( P K P ) ∣ r ⊥ .
The Hessian upper bound makes Q m ( K ) Q_m(K) Q m ( K ) a bounded multiplication operator
for each fixed rank. The joint graph core therefore extends (4) to the full
form domain: apply it to differences, use positivity from (5) to control
the ordinary gradients, and pass to the limit in the bounded curvature term.
In particular L ⪰ Q m ( K ) ⪰ ( N / m ) a I \mathcal L\succeq Q_m(K)\succeq(N/m)aI L ⪰ Q m ( K ) ⪰ ( N / m ) a I .
The curl t = d 1 I m Y t=d_1I_mY t = d 1 I m Y in the block under consideration is, by (3),
t i j = ( κ i − κ j ) α i α j N m F α , t = − F α m U ( P K r ) . (6) t_{ij}=\frac{(\kappa_i-\kappa_j)\sqrt{\alpha_i\alpha_j}}{\sqrt{Nm}}F_\alpha,
\qquad t=-\frac{F_\alpha}{\sqrt m}U(PKr). \tag{6} t ij = N m ( κ i − κ j ) α i α j F α , t = − m F α U ( P Kr ) . ( 6 ) The denominator comes from two successive single-slot contractions,
a j / N a_j/\sqrt N a j / N and a i / m a_i/\sqrt m a i / m ; no tensor multiplicity is suppressed.
Equations (5)–(6) give
⟨ t , Q m ( K ) − 1 t ⟩ = ∣ F α ∣ 2 N ⟨ P K r , ( ( P K P ) ∣ r ⊥ ) − 1 P K r ⟩ . (7) \langle t,Q_m(K)^{-1}t\rangle
=\frac{|F_\alpha|^2}{N}
\langle PKr,((PKP)|_{r^\perp})^{-1}PKr\rangle. \tag{7} ⟨ t , Q m ( K ) − 1 t ⟩ = N ∣ F α ∣ 2 ⟨ P Kr , (( P K P ) ∣ r ⊥ ) − 1 P Kr ⟩ . ( 7 ) The contribution of this symmetric tensor component to B K B_K B K is
( S / N ) ∣ F α ∣ 2 (S/N)|F_\alpha|^2 ( S / N ) ∣ F α ∣ 2 . Completing the square gives
S − ⟨ P K r , ( ( P K P ) ∣ r ⊥ ) − 1 P K r ⟩ = min w ⊥ r ⟨ r + w , K ( r + w ) ⟩ ≥ a N . (8) S-\langle PKr,((PKP)|_{r^\perp})^{-1}PKr\rangle
=\min_{w\perp r}\langle r+w,K(r+w)\rangle\ge aN. \tag{8} S − ⟨ P Kr , (( P K P ) ∣ r ⊥ ) − 1 P Kr ⟩ = w ⊥ r min ⟨ r + w , K ( r + w )⟩ ≥ a N . ( 8 ) Thus the inverse-curvature cost is at most ( S / N − a ) ∣ F α ∣ 2 (S/N-a)|F_\alpha|^2 ( S / N − a ) ∣ F α ∣ 2 .
This exact cancellation, rather than an estimate on ∥ K ∥ \|K\| ∥ K ∥ , is the
rank-uniform part of the proof.
Projection identity. For clarity we justify the operator identity used to
convert (7) into a projection bound. Let A : X 1 → X 2 A:X_1\to X_2 A : X 1 → X 2 , B : X 2 → X 3 B:X_2\to X_3 B : X 2 → X 3
be closed densely defined with B A = 0 BA=0 B A = 0 including domains. Suppose the closed
form ∥ A ∗ z ∥ 2 + ∥ B z ∥ 2 \|A^*z\|^2+\|Bz\|^2 ∥ A ∗ z ∥ 2 + ∥ B z ∥ 2 represents L ⪰ c I \mathcal L\succeq cI L ⪰ c I , c > 0 c>0 c > 0 .
Then, for u ∈ Dom ( A ) u\in\operatorname{Dom}(A) u ∈ Dom ( A ) ,
∥ ( I − P ker A ) u ∥ 2 = ⟨ A u , L − 1 A u ⟩ . (9) \|(I-P_{\ker A})u\|^2=\langle Au,\mathcal L^{-1}Au\rangle. \tag{9} ∥ ( I − P k e r A ) u ∥ 2 = ⟨ A u , L − 1 A u ⟩ . ( 9 ) Indeed X 2 = ker B ⊕ ( ker B ) ⊥ X_2=\ker B\oplus(\ker B)^\perp X 2 = ker B ⊕ ( ker B ) ⊥ splits the form: the second
summand lies in ker A ∗ \ker A^* ker A ∗ , and the first lies in Dom ( B ) \operatorname{Dom}(B) Dom ( B )
with B = 0 B=0 B = 0 . The corresponding projections preserve both domains. For
z = L − 1 A u z=\mathcal L^{-1}Au z = L − 1 A u , the weak equation tested against the perpendicular
component forces that component to vanish. Testing against all of
Dom ( A ∗ ) \operatorname{Dom}(A^*) Dom ( A ∗ ) (projecting first onto ker B \ker B ker B ) proves
z ∈ Dom ( A A ∗ ) z\in\operatorname{Dom}(AA^*) z ∈ Dom ( A A ∗ ) and A A ∗ z = A u AA^*z=Au A A ∗ z = A u . Thus
A ∗ z = ( I − P ker A ) u A^*z=(I-P_{\ker A})u A ∗ z = ( I − P k e r A ) u , proving (9). If also L ⪰ Q ⪰ c I \mathcal L\succeq Q\succeq cI L ⪰ Q ⪰ c I
with bounded Q Q Q , the form variational formula
⟨ t , L − 1 t ⟩ = sup z { 2 Re ⟨ t , z ⟩ − ℓ ( z ) } ≤ sup z { 2 Re ⟨ t , z ⟩ − ⟨ z , Q z ⟩ } = ⟨ t , Q − 1 t ⟩ (10) \langle t,\mathcal L^{-1}t\rangle
=\sup_z\{2\operatorname{Re}\langle t,z\rangle-\ell(z)\}
\le\sup_z\{2\operatorname{Re}\langle t,z\rangle-\langle z,Qz\rangle\}
=\langle t,Q^{-1}t\rangle \tag{10} ⟨ t , L − 1 t ⟩ = z sup { 2 Re ⟨ t , z ⟩ − ℓ ( z )} ≤ z sup { 2 Re ⟨ t , z ⟩ − ⟨ z , Q z ⟩} = ⟨ t , Q − 1 t ⟩ ( 10 ) has its first supremum over the form domain and its second over X 2 X_2 X 2 .
Apply (9)–(10) to A = d 1 A=d_1 A = d 1 , B = d 2 B=d_2 B = d 2 , u = I m Y u=I_mY u = I m Y , and Q = Q m ( K ) Q=Q_m(K) Q = Q m ( K ) .
The isometry I m I_m I m identifies the kernel projection with P C m P_{C_m} P C m .
Sum (7)–(8) over blocks, integrate, and substitute in (2). This yields
∥ D m ∗ F ∥ 2 2 ≥ ∥ ∇ F ∥ 2 2 + a ∥ F ∥ 2 2 \|D_m^*F\|_2^2\ge\|\nabla F\|_2^2+a\|F\|_2^2 ∥ D m ∗ F ∥ 2 2 ≥ ∥∇ F ∥ 2 2 + a ∥ F ∥ 2 2 on the potential core.
For general F ∈ Dom ( D m ∗ ) F\in\operatorname{Dom}(D_m^*) F ∈ Dom ( D m ∗ ) , the proved graph core gives
F k → F F_k\to F F k → F and D m ∗ F k → D m ∗ F D_m^*F_k\to D_m^*F D m ∗ F k → D m ∗ F . Apply the core estimate to
F k − F l F_k-F_l F k − F l to see ∇ F k \nabla F_k ∇ F k is Cauchy. The closed distributional derivative
then gives F ∈ W 1 , 2 F\in W^{1,2} F ∈ W 1 , 2 and ∇ F k → ∇ F \nabla F_k\to\nabla F ∇ F k → ∇ F . Passing to the
limit proves the theorem, including its domain assertion.