Each result cited is universally quantified over the data in its own statement.
Throughout, H = H − 3 H=H^{-3} H = H − 3 and V = H − 2 V=H^{-2} V = H − 2 carry the inner products of orders − 3 -3 − 3 and − 2 -2 − 2 (The Wick-Square Problem on the Sobolev Triple of Order Two: Standing Notation §triple ); by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §domain , D ( A ) = H − 1 D(A)=H^{-1} D ( A ) = H − 1 , A x Ax A x is the family k ↦ μ k x ( k ) k\mapsto\mu_{k}x(k) k ↦ μ k x ( k ) and ∣ A x ∣ H = ∣ x ∣ H − 1 |Ax|_{H}=|x|_{H^{-1}} ∣ A x ∣ H = ∣ x ∣ H − 1 for x ∈ H − 1 x\in H^{-1} x ∈ H − 1 ; in particular A A A is linear, since the vector operations on families are modewise. Elementary arithmetic in R \mathbb{R} R (rearrangement, the triangle inequality, monotonicity of squares of nonnegative numbers, the limit laws and the order of limits) is used without further mention under The Real Numbers: Standing Notation and Background §background , and the Cauchy-Schwarz inequality The Cauchy-Schwarz Inequality in a Real Inner Product Space in H H H , V V V and H − 1 H^{-1} H − 1 under Real Hilbert Spaces: Standing Notation and Background §background . Lattice sums are manipulated with Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §linear , Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §nonnegative and Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §comparison . We fix two tools. Since 1 ≤ μ k 1\le\mu_{k} 1 ≤ μ k (The Wick-Square Problem on the Torus: Standing Notation §modes ), μ k m ≤ μ k m ′ \mu_{k}^{m}\le\mu_{k}^{m'} μ k m ≤ μ k m ′ for natural numbers m ≤ m ′ m\le m' m ≤ m ′ ; and since 0 < q k 0<q_{k} 0 < q k by The Riccati Coefficients of the Wick-Square Problem: Existence, the Gaussian Profile and Summable Constants §root and q k ≤ β / ( 2 μ k ) q_{k}\le\beta/(2\mu_{k}) q k ≤ β / ( 2 μ k ) by The Riccati Coefficients of the Wick-Square Problem: Existence, the Gaussian Profile and Summable Constants §profile ,
0 < 2 q k ≤ β μ k ≤ β for every k ∈ Z n . (W) 0<2q_{k}\le\frac{\beta}{\mu_{k}}\le\beta\qquad\text{for every }k\in\mathbb{Z}^{n}.\qquad\text{(W)} 0 < 2 q k ≤ μ k β ≤ β for every k ∈ Z n . (W)
Further, by Lattice Sums of the Fourier Weights of the Torus, and the Negative Sobolev Norms as Lattice Sums §sobolev , for m ∈ { 1 , 2 , 3 } m\in\{1,2,3\} m ∈ { 1 , 2 , 3 } a family c c c lies in H − m H^{-m} H − m exactly when k ↦ c ( k ) 2 / μ k m k\mapsto c(k)^{2}/\mu_{k}^{m} k ↦ c ( k ) 2 / μ k m is cube-summable, and then ∣ c ∣ H − m 2 |c|_{H^{-m}}^{2} ∣ c ∣ H − m 2 is its lattice sum; we refer to this as (S). For m = 2 m=2 m = 2 and m = 3 m=3 m = 3 these are V V V and H H H with their norms.
Step 1 (The Riccati drift and the gradient form). (a) Let y , y ′ ∈ V y,y'\in V y , y ′ ∈ V . By The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §drift , B q y B_{q}y B q y is the family k ↦ 2 q k y ( k ) k\mapsto2q_{k}y(k) k ↦ 2 q k y ( k ) , so B q y − B q y ′ = B q ( y − y ′ ) B_{q}y-B_{q}y'=B_{q}(y-y') B q y − B q y ′ = B q ( y − y ′ ) . For m ∈ { 2 , 3 } m\in\{2,3\} m ∈ { 2 , 3 } , (W) gives ( 2 q k y ( k ) ) 2 / μ k m ≤ β 2 y ( k ) 2 / μ k m (2q_{k}y(k))^{2}/\mu_{k}^{m}\le\beta^{2}y(k)^{2}/\mu_{k}^{m} ( 2 q k y ( k ) ) 2 / μ k m ≤ β 2 y ( k ) 2 / μ k m , and by (S) the family k ↦ y ( k ) 2 / μ k m k\mapsto y(k)^{2}/\mu_{k}^{m} k ↦ y ( k ) 2 / μ k m is cube-summable with lattice sum ∣ y ∣ V 2 |y|_{V}^{2} ∣ y ∣ V 2 for m = 2 m=2 m = 2 and ∣ y ∣ H 2 |y|_{H}^{2} ∣ y ∣ H 2 for m = 3 m=3 m = 3 (recall V ⊆ H V\subseteq H V ⊆ H ). By comparison and (S) again, B q y ∈ V B_{q}y\in V B q y ∈ V and
∣ B q y ∣ V ≤ β ∣ y ∣ V , ∣ B q y ∣ H ≤ β ∣ y ∣ H . |B_{q}y|_{V}\le\beta\,|y|_{V},\qquad|B_{q}y|_{H}\le\beta\,|y|_{H}. ∣ B q y ∣ V ≤ β ∣ y ∣ V , ∣ B q y ∣ H ≤ β ∣ y ∣ H .
(b) Let y ∈ H − 1 y\in H^{-1} y ∈ H − 1 and v ∈ V v\in V v ∈ V . By Hilbert Triples: Standing Notation and Background §operator , ⟨ A y , v ⟩ H = ⟨ y , v ⟩ V \langle Ay,v\rangle_{H}=\langle y,v\rangle_{V} ⟨ A y , v ⟩ H = ⟨ y , v ⟩ V . Taking v = y v=y v = y and using Cauchy-Schwarz in H H H ,
∣ y ∣ V 2 = ⟨ A y , y ⟩ H ≤ ∣ y ∣ H − 1 ∣ y ∣ H . |y|_{V}^{2}=\langle Ay,y\rangle_{H}\le|y|_{H^{-1}}\,|y|_{H}. ∣ y ∣ V 2 = ⟨ A y , y ⟩ H ≤ ∣ y ∣ H − 1 ∣ y ∣ H .
(c) Let y ∈ H − 1 y\in H^{-1} y ∈ H − 1 and b ∈ H b\in H b ∈ H . Let x x x be the family k ↦ b ( k ) / μ k 3 k\mapsto b(k)/\mu_{k}^{3} k ↦ b ( k ) / μ k 3 . Since x ( k ) 2 / μ k = b ( k ) 2 / μ k 7 ≤ b ( k ) 2 / μ k 3 x(k)^{2}/\mu_{k}=b(k)^{2}/\mu_{k}^{7}\le b(k)^{2}/\mu_{k}^{3} x ( k ) 2 / μ k = b ( k ) 2 / μ k 7 ≤ b ( k ) 2 / μ k 3 and b ∈ H b\in H b ∈ H , (S) and comparison give x ∈ H − 1 x\in H^{-1} x ∈ H − 1 and ∣ x ∣ H − 1 ≤ ∣ b ∣ H |x|_{H^{-1}}\le|b|_{H} ∣ x ∣ H − 1 ≤ ∣ b ∣ H . By the first statement of The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings , ⟨ A y , e k ⟩ H = μ k y ( k ) / μ k 3 \langle Ay,e_{k}\rangle_{H}=\mu_{k}y(k)/\mu_{k}^{3} ⟨ A y , e k ⟩ H = μ k y ( k ) / μ k 3 and ⟨ b , e k ⟩ H = b ( k ) / μ k 3 \langle b,e_{k}\rangle_{H}=b(k)/\mu_{k}^{3} ⟨ b , e k ⟩ H = b ( k ) / μ k 3 , so by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §gradient-form G ( A y , b ) G(Ay,b) G ( A y , b ) is the lattice sum of k ↦ y ( k ) b ( k ) / μ k 5 k\mapsto y(k)b(k)/\mu_{k}^{5} k ↦ y ( k ) b ( k ) / μ k 5 ; by the last statement of The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings , applied to x ∈ H − 1 x\in H^{-1} x ∈ H − 1 and y ∈ H y\in H y ∈ H , so is ⟨ A x , y ⟩ H \langle Ax,y\rangle_{H} ⟨ A x , y ⟩ H . Hence G ( A y , b ) = ⟨ A x , y ⟩ H G(Ay,b)=\langle Ax,y\rangle_{H} G ( A y , b ) = ⟨ A x , y ⟩ H , and by Cauchy-Schwarz
∣ G ( A y , b ) ∣ ≤ ∣ A x ∣ H ∣ y ∣ H = ∣ x ∣ H − 1 ∣ y ∣ H ≤ ∣ b ∣ H ∣ y ∣ H . |G(Ay,b)|\le|Ax|_{H}\,|y|_{H}=|x|_{H^{-1}}\,|y|_{H}\le|b|_{H}\,|y|_{H}. ∣ G ( A y , b ) ∣ ≤ ∣ A x ∣ H ∣ y ∣ H = ∣ x ∣ H − 1 ∣ y ∣ H ≤ ∣ b ∣ H ∣ y ∣ H .
(d) By The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §gradient-form , 0 S y m ⪯ G ⪯ I H 0_{\mathrm{Sym}}\preceq G\preceq I_{H} 0 Sym ⪯ G ⪯ I H , so 0 ≤ G ( v , v ) ≤ ∣ v ∣ H 2 0\le G(v,v)\le|v|_{H}^{2} 0 ≤ G ( v , v ) ≤ ∣ v ∣ H 2 for v ∈ H v\in H v ∈ H ; by Elementary Properties of Bounded Symmetric Bilinear Forms: Norm, Quadratic Form, Order and Continuity §quadratic-norm , ∥ G ∥ ≤ 1 \lVert G\rVert\le1 ∥ G ∥ ≤ 1 , whence ∣ G ( v , v ′ ) ∣ ≤ ∣ v ∣ H ∣ v ′ ∣ H |G(v,v')|\le|v|_{H}|v'|_{H} ∣ G ( v , v ′ ) ∣ ≤ ∣ v ∣ H ∣ v ′ ∣ H for v , v ′ ∈ H v,v'\in H v , v ′ ∈ H by Elementary Properties of Bounded Symmetric Bilinear Forms: Norm, Quadratic Form, Order and Continuity §bound . By bilinearity and symmetry, G ( v , v ) − G ( v ′ , v ′ ) = G ( v − v ′ , v + v ′ ) G(v,v)-G(v',v')=G(v-v',v+v') G ( v , v ) − G ( v ′ , v ′ ) = G ( v − v ′ , v + v ′ ) , and G ( v + v ′ , v + v ′ ) + G ( v − v ′ , v − v ′ ) = 2 G ( v , v ) + 2 G ( v ′ , v ′ ) G(v+v',v+v')+G(v-v',v-v')=2G(v,v)+2G(v',v') G ( v + v ′ , v + v ′ ) + G ( v − v ′ , v − v ′ ) = 2 G ( v , v ) + 2 G ( v ′ , v ′ ) ; as both terms on the left are nonnegative, G ( v ± v ′ , v ± v ′ ) ≤ 2 G ( v , v ) + 2 G ( v ′ , v ′ ) G(v\pm v',v\pm v')\le2G(v,v)+2G(v',v') G ( v ± v ′ , v ± v ′ ) ≤ 2 G ( v , v ) + 2 G ( v ′ , v ′ ) .
Step 2 (The free solution minus the penalty). Put A 0 = ∑ k ∈ Z n a k A_{0}=\sum_{k\in\mathbb{Z}^{n}}a_{k} A 0 = ∑ k ∈ Z n a k , which exists by The Riccati Coefficients of the Wick-Square Problem: Existence, the Gaussian Profile and Summable Constants §constants , let η 0 ( k ) = q k − β / ( 2 μ k ) \eta_{0}(k)=q_{k}-\beta/(2\mu_{k}) η 0 ( k ) = q k − β / ( 2 μ k ) , and let c 0 : H − 3 → R c_{0}:H^{-3}\to\mathbb{R} c 0 : H − 3 → R be the constant function with value A 0 A_{0} A 0 . By The Riccati Coefficients of the Wick-Square Problem: Existence, the Gaussian Profile and Summable Constants §profile , μ k 2 ∣ η 0 ( k ) ∣ = μ k 2 ( β / ( 2 μ k ) − q k ) ≤ ( β γ + β 2 ) / 4 \mu_{k}^{2}|\eta_{0}(k)|=\mu_{k}^{2}(\beta/(2\mu_{k})-q_{k})\le(\beta\gamma+\beta^{2})/4 μ k 2 ∣ η 0 ( k ) ∣ = μ k 2 ( β / ( 2 μ k ) − q k ) ≤ ( β γ + β 2 ) /4 , so η 0 \eta_{0} η 0 is a curvature family with this bound. Since c 0 ( x ) = ⟨ 0 , x ⟩ H − 3 + A 0 c_{0}(x)=\langle0,x\rangle_{H^{-3}}+A_{0} c 0 ( x ) = ⟨ 0 , x ⟩ H − 3 + A 0 and H − 3 H^{-3} H − 3 is a real Hilbert space (The Negative-Order Sobolev Spaces of the Torus are Hilbert Spaces: the Embedding of the Square-Integrable Classes, the Rescaled Trigonometric Basis, the Series Form of the Inner Product and the Inclusion of the Scale §hilbert ), Affine and Quadratic Functions on a Real Hilbert Space are of Class C 2 C^2 C 2 §affine gives that c 0 c_{0} c 0 is of class C 2 C^{2} C 2 on H − 3 H^{-3} H − 3 with D c 0 ( x ) = 0 Dc_{0}(x)=0 D c 0 ( x ) = 0 for every x x x . Let x ∈ H − 1 x\in H^{-1} x ∈ H − 1 . The families k ↦ q k x ( k ) 2 + a k k\mapsto q_{k}x(k)^{2}+a_{k} k ↦ q k x ( k ) 2 + a k (The Galerkin Solutions of the Wick-Square Problem Converge to a Classical Solution of the Renormalised Equation, while the Bare Solutions Diverge §limit ), k ↦ a k k\mapsto a_{k} k ↦ a k and k ↦ β x ( k ) 2 / ( 2 μ k ) k\mapsto\beta x(k)^{2}/(2\mu_{k}) k ↦ β x ( k ) 2 / ( 2 μ k ) (The Gaussian Penalty of the Wick-Square Problem and linearity) are cube-summable, so by linearity so is k ↦ η 0 ( k ) x ( k ) 2 k\mapsto\eta_{0}(k)x(k)^{2} k ↦ η 0 ( k ) x ( k ) 2 , their combination, and
u 0 ( x ) − P ( x ) = ∑ k ∈ Z n η 0 ( k ) x ( k ) 2 + c 0 ( x ) . u_{0}(x)-P(x)=\sum_{k\in\mathbb{Z}^{n}}\eta_{0}(k)\,x(k)^{2}+c_{0}(x). u 0 ( x ) − P ( x ) = k ∈ Z n ∑ η 0 ( k ) x ( k ) 2 + c 0 ( x ) .
Thus ψ 0 = u 0 − P \psi_{0}=u_{0}-P ψ 0 = u 0 − P is regular (Regular Functions for the Wick-Square Problem: Diagonal Quadratics of Curvature of Order the Inverse Squared Weight, plus Twice Differentiable Functions on the Sobolev Space of Order -3 ), with curvature family η 0 \eta_{0} η 0 and weak part c 0 c_{0} c 0 . By Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §derivatives , ∂ k ψ 0 ( x ) = 2 η 0 ( k ) x ( k ) \partial_{k}\psi_{0}(x)=2\eta_{0}(k)x(k) ∂ k ψ 0 ( x ) = 2 η 0 ( k ) x ( k ) . By The Cutoff Wick Square is Minus the Free-Field Generator of the Gaussian Penalty, and the Penalised Form of the Cutoff Operators §derivatives , P P P is twice differentiable along the modes with ∂ k P ( x ) = β x ( k ) / μ k \partial_{k}P(x)=\beta x(k)/\mu_{k} ∂ k P ( x ) = β x ( k ) / μ k . Since u 0 = P + ψ 0 u_{0}=P+\psi_{0} u 0 = P + ψ 0 pointwise on H − 1 H^{-1} H − 1 , Mode Derivatives of Linear Combinations and of Restrictions of Twice Differentiable Functions on a Negative Sobolev Space §linear gives, for all x ∈ H − 1 x\in H^{-1} x ∈ H − 1 and k ∈ Z n k\in\mathbb{Z}^{n} k ∈ Z n ,
∂ k u 0 ( x ) = β x ( k ) μ k + 2 q k x ( k ) − β x ( k ) μ k = 2 q k x ( k ) . \partial_{k}u_{0}(x)=\frac{\beta x(k)}{\mu_{k}}+2q_{k}x(k)-\frac{\beta x(k)}{\mu_{k}}=2q_{k}\,x(k). ∂ k u 0 ( x ) = μ k β x ( k ) + 2 q k x ( k ) − μ k β x ( k ) = 2 q k x ( k ) .
Step 3 (Clause 1). Let χ \chi χ be regular, with a curvature family η \eta η , curvature bound C χ C_{\chi} C χ and weak part ϕ \phi ϕ . By Step 2 and Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §linear , u 0 + χ − P = ψ 0 + χ u_{0}+\chi-P=\psi_{0}+\chi u 0 + χ − P = ψ 0 + χ is regular. By Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §derivatives , χ \chi χ is twice differentiable along the modes, and so is u 0 u_{0} u 0 by The Galerkin Solutions of the Wick-Square Problem Converge to a Classical Solution of the Renormalised Equation, while the Bare Solutions Diverge §solution ; hence so is u 0 + χ u_{0}+\chi u 0 + χ , with ∂ k ( u 0 + χ ) = ∂ k u 0 + ∂ k χ \partial_{k}(u_{0}+\chi)=\partial_{k}u_{0}+\partial_{k}\chi ∂ k ( u 0 + χ ) = ∂ k u 0 + ∂ k χ and likewise for the second derivatives and for ψ 0 + χ \psi_{0}+\chi ψ 0 + χ (Mode Derivatives of Linear Combinations and of Restrictions of Twice Differentiable Functions on a Negative Sobolev Space §linear ). Fix x ∈ H − 1 x\in H^{-1} x ∈ H − 1 . By Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §generator , L χ L\chi L χ is defined at x x x ; by Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §gradient with θ = 0 \theta=0 θ = 0 , ∣ D χ ( x ) ∣ 2 |D\chi(x)|^{2} ∣ Dχ ( x ) ∣ 2 is defined.
Cross term. Put z = D ϕ ( x ) ∈ H − 3 = H z=D\phi(x)\in H^{-3}=H z = D ϕ ( x ) ∈ H − 3 = H . By Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §derivatives and the first statement of The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings , ∂ k χ ( x ) = 2 η ( k ) x ( k ) + z ( k ) / μ k 3 \partial_{k}\chi(x)=2\eta(k)x(k)+z(k)/\mu_{k}^{3} ∂ k χ ( x ) = 2 η ( k ) x ( k ) + z ( k ) / μ k 3 , so 2 q k x ( k ) ∂ k χ ( x ) 2q_{k}x(k)\partial_{k}\chi(x) 2 q k x ( k ) ∂ k χ ( x ) is the sum of 4 q k η ( k ) x ( k ) 2 4q_{k}\eta(k)x(k)^{2} 4 q k η ( k ) x ( k ) 2 and 2 q k x ( k ) z ( k ) / μ k 3 2q_{k}x(k)z(k)/\mu_{k}^{3} 2 q k x ( k ) z ( k ) / μ k 3 . By (W) and ∣ η ( k ) ∣ ≤ C χ / μ k 2 |\eta(k)|\le C_{\chi}/\mu_{k}^{2} ∣ η ( k ) ∣ ≤ C χ / μ k 2 , the first has absolute value at most 2 β C χ x ( k ) 2 / μ k 2\beta C_{\chi}x(k)^{2}/\mu_{k} 2 β C χ x ( k ) 2 / μ k , a cube-summable family by The Wick-Square Problem on the Torus: Standing Notation §state-space ; by (W), the second has absolute value at most β ∣ x ( k ) z ( k ) ∣ / μ k 2 \beta|x(k)z(k)|/\mu_{k}^{2} β ∣ x ( k ) z ( k ) ∣/ μ k 2 , cube-summable by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings . By comparison and linearity, k ↦ 2 q k x ( k ) ∂ k χ ( x ) k\mapsto2q_{k}x(k)\partial_{k}\chi(x) k ↦ 2 q k x ( k ) ∂ k χ ( x ) is cube-summable.
The identity. Let F N F_{N} F N be the Wick-ordered cutoff operators for the running cost g ∣ H − 1 g|_{H^{-1}} g ∣ H − 1 , and F ~ N \widetilde{F}_{N} F N , D ~ \widetilde{\mathcal{D}} D , F ~ \widetilde{F} F the Wick-ordered cutoff operators, the domain and the renormalised operator for the zero running cost. By The Cutoff Wick Square is Minus the Free-Field Generator of the Gaussian Penalty, and the Penalised Form of the Cutoff Operators §penalised , for every N ∈ N N\in\mathbb{N} N ∈ N ,
F N [ u 0 + χ ] ( x ) = γ ( u 0 + χ ) ( x ) − L N ( ψ 0 + χ ) ( x ) + 1 2 ∣ D N ( u 0 + χ ) ( x ) ∣ 2 − g ( x ) , F_{N}[u_{0}+\chi](x)=\gamma\,(u_{0}+\chi)(x)-L_{N}(\psi_{0}+\chi)(x)+\tfrac12|D_{N}(u_{0}+\chi)(x)|^{2}-g(x), F N [ u 0 + χ ] ( x ) = γ ( u 0 + χ ) ( x ) − L N ( ψ 0 + χ ) ( x ) + 2 1 ∣ D N ( u 0 + χ ) ( x ) ∣ 2 − g ( x ) ,
F ~ N [ u 0 ] ( x ) = γ u 0 ( x ) − L N ψ 0 ( x ) + 1 2 ∣ D N u 0 ( x ) ∣ 2 . \widetilde{F}_{N}[u_{0}](x)=\gamma\,u_{0}(x)-L_{N}\psi_{0}(x)+\tfrac12|D_{N}u_{0}(x)|^{2}. F N [ u 0 ] ( x ) = γ u 0 ( x ) − L N ψ 0 ( x ) + 2 1 ∣ D N u 0 ( x ) ∣ 2 .
By the additivity of mode derivatives and the definitions The Free-Field Generator with a Mode Cutoff §generator and The Gradient Energy with a Mode Cutoff §gradient (finite sums over Γ N \Gamma_{N} Γ N ), L N ( ψ 0 + χ ) ( x ) = L N ψ 0 ( x ) + L N χ ( x ) L_{N}(\psi_{0}+\chi)(x)=L_{N}\psi_{0}(x)+L_{N}\chi(x) L N ( ψ 0 + χ ) ( x ) = L N ψ 0 ( x ) + L N χ ( x ) , and by Step 2
1 2 ∣ D N ( u 0 + χ ) ( x ) ∣ 2 − 1 2 ∣ D N u 0 ( x ) ∣ 2 = ∑ k ∈ Γ N 1 2 ( 2 ∂ k u 0 ( x ) ∂ k χ ( x ) + ( ∂ k χ ( x ) ) 2 ) = ∑ k ∈ Γ N 2 q k x ( k ) ∂ k χ ( x ) + 1 2 ∣ D N χ ( x ) ∣ 2 . \tfrac12|D_{N}(u_{0}+\chi)(x)|^{2}-\tfrac12|D_{N}u_{0}(x)|^{2}=\sum_{k\in\Gamma_{N}}\tfrac12\bigl(2\,\partial_{k}u_{0}(x)\,\partial_{k}\chi(x)+(\partial_{k}\chi(x))^{2}\bigr)=\sum_{k\in\Gamma_{N}}2q_{k}x(k)\,\partial_{k}\chi(x)+\tfrac12|D_{N}\chi(x)|^{2}. 2 1 ∣ D N ( u 0 + χ ) ( x ) ∣ 2 − 2 1 ∣ D N u 0 ( x ) ∣ 2 = k ∈ Γ N ∑ 2 1 ( 2 ∂ k u 0 ( x ) ∂ k χ ( x ) + ( ∂ k χ ( x ) ) 2 ) = k ∈ Γ N ∑ 2 q k x ( k ) ∂ k χ ( x ) + 2 1 ∣ D N χ ( x ) ∣ 2 .
Subtracting,
F N [ u 0 + χ ] ( x ) = F ~ N [ u 0 ] ( x ) + γ χ ( x ) − L N χ ( x ) + ∑ k ∈ Γ N 2 q k x ( k ) ∂ k χ ( x ) + 1 2 ∣ D N χ ( x ) ∣ 2 − g ( x ) . F_{N}[u_{0}+\chi](x)=\widetilde{F}_{N}[u_{0}](x)+\gamma\,\chi(x)-L_{N}\chi(x)+\sum_{k\in\Gamma_{N}}2q_{k}x(k)\,\partial_{k}\chi(x)+\tfrac12|D_{N}\chi(x)|^{2}-g(x). F N [ u 0 + χ ] ( x ) = F N [ u 0 ] ( x ) + γ χ ( x ) − L N χ ( x ) + k ∈ Γ N ∑ 2 q k x ( k ) ∂ k χ ( x ) + 2 1 ∣ D N χ ( x ) ∣ 2 − g ( x ) .
As N → ∞ N\to\infty N → ∞ : F ~ N [ u 0 ] ( x ) → 0 \widetilde{F}_{N}[u_{0}](x)\to0 F N [ u 0 ] ( x ) → 0 , because ( u 0 , x ) ∈ D ~ (u_{0},x)\in\widetilde{\mathcal{D}} ( u 0 , x ) ∈ D and F ~ [ u 0 ] ( x ) = 0 \widetilde{F}[u_{0}](x)=0 F [ u 0 ] ( x ) = 0 by The Galerkin Solutions of the Wick-Square Problem Converge to a Classical Solution of the Renormalised Equation, while the Bare Solutions Diverge §solution (with u 0 = R u_{0}=R u 0 = R by The Wick-Square Problem on the Sobolev Triple of Order Two: Standing Notation §free ) and The Renormalised Hamilton-Jacobi-Bellman Operator of the Wick-Square Problem as the Limit of the Wick-Ordered Cutoff Operators §operator ; L N χ ( x ) → L χ ( x ) L_{N}\chi(x)\to L\chi(x) L N χ ( x ) → L χ ( x ) and ∣ D N χ ( x ) ∣ 2 → ∣ D χ ( x ) ∣ 2 |D_{N}\chi(x)|^{2}\to|D\chi(x)|^{2} ∣ D N χ ( x ) ∣ 2 → ∣ Dχ ( x ) ∣ 2 by The Free-Field Generator with a Mode Cutoff §limit and The Gradient Energy with a Mode Cutoff §limit ; and the cube sums of the cross family converge to its lattice sum. By the limit laws, ( F N [ u 0 + χ ] ( x ) ) N (F_{N}[u_{0}+\chi](x))_{N} ( F N [ u 0 + χ ] ( x ) ) N converges, so ( u 0 + χ , x ) ∈ D (u_{0}+\chi,x)\in\mathcal{D} ( u 0 + χ , x ) ∈ D (The Renormalised Hamilton-Jacobi-Bellman Operator of the Wick-Square Problem as the Limit of the Wick-Ordered Cutoff Operators §domain ), and its limit F [ u 0 + χ ] ( x ) F[u_{0}+\chi](x) F [ u 0 + χ ] ( x ) is the right-hand side of clause 1.
Step 4 (Clause 2). Let φ ∈ C 2 ( H ) \varphi\in C^{2}(H) φ ∈ C 2 ( H ) , c ∈ R c\in\mathbb{R} c ∈ R and χ = ( φ + c h ) ∣ H − 1 \chi=(\varphi+c\,h)|_{H^{-1}} χ = ( φ + c h ) ∣ H − 1 . As H H H is H − 3 H^{-3} H − 3 with its inner product and C 2 ( H ) C^{2}(H) C 2 ( H ) is the class of The Classes C 1 C^1 C 1 and C 2 C^2 C 2 on an Open Subset of a Real Inner Product Space §c2 for that space (Hilbert Triples: Standing Notation and Background §open-sets , Real Hilbert Spaces: Series, Products, Orthonormal Bases and Differential Calculus §calculus ), φ \varphi φ is of class C 2 C^{2} C 2 on H − 3 H^{-3} H − 3 , with gradient map D φ D\varphi D φ and Hessian map D 2 φ D^{2}\varphi D 2 φ . Put η c ( k ) = c / ( 2 μ k 2 ) \eta_{c}(k)=c/(2\mu_{k}^{2}) η c ( k ) = c / ( 2 μ k 2 ) , so μ k 2 ∣ η c ( k ) ∣ = ∣ c ∣ / 2 \mu_{k}^{2}|\eta_{c}(k)|=|c|/2 μ k 2 ∣ η c ( k ) ∣ = ∣ c ∣/2 . For x ∈ H − 1 ⊆ V x\in H^{-1}\subseteq V x ∈ H − 1 ⊆ V , (S) with m = 2 m=2 m = 2 and linearity give c h ( x ) = c 2 ∣ x ∣ V 2 = ∑ k ∈ Z n η c ( k ) x ( k ) 2 c\,h(x)=\tfrac{c}{2}|x|_{V}^{2}=\sum_{k\in\mathbb{Z}^{n}}\eta_{c}(k)x(k)^{2} c h ( x ) = 2 c ∣ x ∣ V 2 = ∑ k ∈ Z n η c ( k ) x ( k ) 2 , so χ ( x ) = ∑ k η c ( k ) x ( k ) 2 + φ ( x ) \chi(x)=\sum_{k}\eta_{c}(k)x(k)^{2}+\varphi(x) χ ( x ) = ∑ k η c ( k ) x ( k ) 2 + φ ( x ) : χ \chi χ is regular with curvature family η c \eta_{c} η c and weak part φ \varphi φ .
Fix x ∈ H − 1 = D ( A ) x\in H^{-1}=D(A) x ∈ H − 1 = D ( A ) , and put p = D φ ( x ) + c A x ∈ H p=D\varphi(x)+c\,Ax\in H p = D φ ( x ) + c A x ∈ H and X = D 2 φ ( x ) ∣ V + c I V ∈ S y m ( V ) X=D^{2}\varphi(x)|_{V}+c\,I_{V}\in\mathrm{Sym}(V) X = D 2 φ ( x ) ∣ V + c I V ∈ Sym ( V ) . By Regular Functions: Mode Derivatives, the Free-Field Generator, the Gradient Energy, the Renormalised Operator at the Gaussian Penalty plus a Regular Function, and Linear Combinations §derivatives ,
∂ k χ ( x ) = c x ( k ) μ k 2 + ⟨ D φ ( x ) , e k ⟩ H , ∂ k 2 χ ( x ) = c μ k 2 + D 2 φ ( x ) ( e k , e k ) . \partial_{k}\chi(x)=\frac{c\,x(k)}{\mu_{k}^{2}}+\langle D\varphi(x),e_{k}\rangle_{H},\qquad\partial_{k}^{2}\chi(x)=\frac{c}{\mu_{k}^{2}}+D^{2}\varphi(x)(e_{k},e_{k}). ∂ k χ ( x ) = μ k 2 c x ( k ) + ⟨ D φ ( x ) , e k ⟩ H , ∂ k 2 χ ( x ) = μ k 2 c + D 2 φ ( x ) ( e k , e k ) .
By The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings , ⟨ A x , e k ⟩ H = μ k x ( k ) / μ k 3 = x ( k ) / μ k 2 \langle Ax,e_{k}\rangle_{H}=\mu_{k}x(k)/\mu_{k}^{3}=x(k)/\mu_{k}^{2} ⟨ A x , e k ⟩ H = μ k x ( k ) / μ k 3 = x ( k ) / μ k 2 ; by linearity of the inner product,
∂ k χ ( x ) = ⟨ p , e k ⟩ H = p ( k ) μ k 3 . (4.1) \partial_{k}\chi(x)=\langle p,e_{k}\rangle_{H}=\frac{p(k)}{\mu_{k}^{3}}.\qquad\text{(4.1)} ∂ k χ ( x ) = ⟨ p , e k ⟩ H = μ k 3 p ( k ) . (4.1)
Since e k ∈ V e_{k}\in V e k ∈ V and I V ( e k , e k ) = ∣ e k ∣ V 2 = 1 / μ k 2 I_{V}(e_{k},e_{k})=|e_{k}|_{V}^{2}=1/\mu_{k}^{2} I V ( e k , e k ) = ∣ e k ∣ V 2 = 1/ μ k 2 (Lattice Sums of the Fourier Weights of the Torus, and the Negative Sobolev Norms as Lattice Sums §units with m = 2 m=2 m = 2 ), the definitions of restriction and of sums of forms (Bounded Symmetric Bilinear Forms on a Real Inner Product Space: Norm, Order, Identity Form and Restriction §restriction , Bounded Symmetric Bilinear Forms on a Real Inner Product Space: Norm, Order, Identity Form and Restriction §identity ) give
∂ k 2 χ ( x ) = X ( e k , e k ) . (4.2) \partial_{k}^{2}\chi(x)=X(e_{k},e_{k}).\qquad\text{(4.2)} ∂ k 2 χ ( x ) = X ( e k , e k ) . (4.2)
Gradient energy: by (4.1), ∣ D N χ ( x ) ∣ 2 |D_{N}\chi(x)|^{2} ∣ D N χ ( x ) ∣ 2 is the N N N th cube sum of k ↦ ⟨ p , e k ⟩ H 2 k\mapsto\langle p,e_{k}\rangle_{H}^{2} k ↦ ⟨ p , e k ⟩ H 2 , whose lattice sum is G ( p , p ) G(p,p) G ( p , p ) by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §gradient-form ; so ∣ D χ ( x ) ∣ 2 = G ( p , p ) |D\chi(x)|^{2}=G(p,p) ∣ Dχ ( x ) ∣ 2 = G ( p , p ) . Generator: by (4.1) and (4.2), μ k x ( k ) ∂ k χ ( x ) = x ( k ) p ( k ) / μ k 2 \mu_{k}x(k)\partial_{k}\chi(x)=x(k)p(k)/\mu_{k}^{2} μ k x ( k ) ∂ k χ ( x ) = x ( k ) p ( k ) / μ k 2 and L N χ ( x ) L_{N}\chi(x) L N χ ( x ) is ν 2 \tfrac{\nu}{2} 2 ν times the N N N th cube sum of k ↦ X ( e k , e k ) k\mapsto X(e_{k},e_{k}) k ↦ X ( e k , e k ) minus that of k ↦ x ( k ) p ( k ) / μ k 2 k\mapsto x(k)p(k)/\mu_{k}^{2} k ↦ x ( k ) p ( k ) / μ k 2 ; by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §noise and The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings these converge to T r f X \mathrm{Tr}_{f}X Tr f X and ⟨ A x , p ⟩ H \langle Ax,p\rangle_{H} ⟨ A x , p ⟩ H , so L χ ( x ) = ν 2 T r f X − ⟨ A x , p ⟩ H L\chi(x)=\tfrac{\nu}{2}\mathrm{Tr}_{f}X-\langle Ax,p\rangle_{H} L χ ( x ) = 2 ν Tr f X − ⟨ A x , p ⟩ H . Cross term: let x ′ x' x ′ be the family k ↦ 2 q k x ( k ) / μ k k\mapsto2q_{k}x(k)/\mu_{k} k ↦ 2 q k x ( k ) / μ k . By (W), x ′ ( k ) 2 / μ k ≤ β 2 x ( k ) 2 / μ k x'(k)^{2}/\mu_{k}\le\beta^{2}x(k)^{2}/\mu_{k} x ′ ( k ) 2 / μ k ≤ β 2 x ( k ) 2 / μ k , so x ′ ∈ H − 1 x'\in H^{-1} x ′ ∈ H − 1 by (S) and comparison, and A x ′ Ax' A x ′ is the family k ↦ 2 q k x ( k ) k\mapsto2q_{k}x(k) k ↦ 2 q k x ( k ) , which is B q x B_{q}x B q x (The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §drift ). By (4.1), 2 q k x ( k ) ∂ k χ ( x ) = x ′ ( k ) p ( k ) / μ k 2 2q_{k}x(k)\partial_{k}\chi(x)=x'(k)p(k)/\mu_{k}^{2} 2 q k x ( k ) ∂ k χ ( x ) = x ′ ( k ) p ( k ) / μ k 2 , whose lattice sum is ⟨ A x ′ , p ⟩ H = ⟨ B q x , p ⟩ H \langle Ax',p\rangle_{H}=\langle B_{q}x,p\rangle_{H} ⟨ A x ′ , p ⟩ H = ⟨ B q x , p ⟩ H by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings . Substituting in the right-hand side of clause 1 and using χ ( x ) = φ ( x ) + c h ( x ) \chi(x)=\varphi(x)+c\,h(x) χ ( x ) = φ ( x ) + c h ( x ) , that right-hand side is
γ ( φ ( x ) + c h ( x ) ) − ν 2 T r f X + 1 2 G ( p , p ) + ⟨ A x + B q x , p ⟩ H − g ( x ) , \gamma\bigl(\varphi(x)+c\,h(x)\bigr)-\tfrac{\nu}{2}\mathrm{Tr}_{f}X+\tfrac12G(p,p)+\langle Ax+B_{q}x,p\rangle_{H}-g(x), γ ( φ ( x ) + c h ( x ) ) − 2 ν Tr f X + 2 1 G ( p , p ) + ⟨ A x + B q x , p ⟩ H − g ( x ) ,
which is F ♯ ( x , φ ( x ) + c h ( x ) , p , X ) F^{\sharp}(x,\varphi(x)+c\,h(x),p,X) F ♯ ( x , φ ( x ) + c h ( x ) , p , X ) by The Shifted Hamilton-Jacobi-Bellman Equation of the Wick-Square Problem on the Sobolev Triple of Order Two §operator .
The shifts. Let δ > 0 \delta>0 δ > 0 . Taking c = δ c=\delta c = δ , the triple form and clause 1 give F [ u 0 + ( φ + δ h ) ∣ H − 1 ] ( x ) = F ♯ ( x , φ ( x ) + δ h ( x ) , D φ ( x ) + δ A x , D 2 φ ( x ) ∣ V + δ I V ) F[u_{0}+(\varphi+\delta h)|_{H^{-1}}](x)=F^{\sharp}(x,\varphi(x)+\delta h(x),D\varphi(x)+\delta Ax,D^{2}\varphi(x)|_{V}+\delta I_{V}) F [ u 0 + ( φ + δ h ) ∣ H − 1 ] ( x ) = F ♯ ( x , φ ( x ) + δ h ( x ) , D φ ( x ) + δ A x , D 2 φ ( x ) ∣ V + δ I V ) , which is F δ ♯ − ( x , φ ( x ) , D φ ( x ) , D 2 φ ( x ) ) F^{\sharp-}_{\delta}(x,\varphi(x),D\varphi(x),D^{2}\varphi(x)) F δ ♯ − ( x , φ ( x ) , D φ ( x ) , D 2 φ ( x )) by Second-Order Equation Operator on an Open Subset of a Hilbert Triple and Its δ \delta δ -Shifts §shifted . Taking c = − δ c=-\delta c = − δ , so that ( φ + c h ) ∣ H − 1 = ( φ − δ h ) ∣ H − 1 (\varphi+c\,h)|_{H^{-1}}=(\varphi-\delta h)|_{H^{-1}} ( φ + c h ) ∣ H − 1 = ( φ − δ h ) ∣ H − 1 , c A x = − δ A x c\,Ax=-\delta Ax c A x = − δ A x and c I V = − δ I V c\,I_{V}=-\delta I_{V} c I V = − δ I V (Bounded Symmetric Bilinear Forms on a Real Inner Product Space: Norm, Order, Identity Form and Restriction §identity ), the same argument gives the formula for F δ ♯ + F^{\sharp+}_{\delta} F δ ♯ + .
Step 5 (Clauses 3 and 4). We apply A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses to the triple ( H , V , A ) (H,V,A) ( H , V , A ) , which is in the setting of Hilbert Triples: Standing Notation and Background by The Wick-Square Problem on the Sobolev Triple of Order Two: Standing Notation §triple , with: λ 0 = γ \lambda_{0}=\gamma λ 0 = γ , positive by The Wick-Square Problem on the Torus: Standing Notation §parameters ; the given C g C_{g} C g and g g g ; ω g ( t ) = ℓ g t \omega_{g}(t)=\ell_{g}t ω g ( t ) = ℓ g t , a modulus of continuity by Linear Moduli of Continuity §modulus , and for x , y ∈ V x,y\in V x , y ∈ V one has ∣ g ( x ) − g ( y ) ∣ ≤ ℓ g ∣ x − y ∣ H ≤ ℓ g ∣ x − y ∣ V |g(x)-g(y)|\le\ell_{g}|x-y|_{H}\le\ell_{g}|x-y|_{V} ∣ g ( x ) − g ( y ) ∣ ≤ ℓ g ∣ x − y ∣ H ≤ ℓ g ∣ x − y ∣ V by Hilbert Triples: Standing Notation and Background §triple ; B = B q B=B_{q} B = B q , a monotone nonlinearity by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §drift ; ℓ = 0 \ell=0 ℓ = 0 and L L L the zero map of H H H , Lipschitz with constant 0 0 0 since d H ( 0 H , 0 H ) = 0 d_{H}(0_{H},0_{H})=0 d H ( 0 H , 0 H ) = 0 , so c L = 0 c_{L}=0 c L = 0 ; Γ = G \Gamma=G Γ = G , with 0 S y m ⪯ G ⪯ I H 0_{\mathrm{Sym}}\preceq G\preceq I_{H} 0 Sym ⪯ G ⪯ I H by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §gradient-form ; ν \nu ν , positive; and f f f , square-summable in V V V by The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §noise . The operator of the proposition is then, at ( x , r , p , X ) ∈ D ( A ) × R × H × S y m ( V ) (x,r,p,X)\in D(A)\times\mathbb{R}\times H\times\mathrm{Sym}(V) ( x , r , p , X ) ∈ D ( A ) × R × H × Sym ( V ) , γ r − ν 2 T r f X + 1 2 G ( p , p ) + ⟨ A x + B q x + 0 H , p ⟩ H − g ( x ) = F ♯ ( x , r , p , X ) \gamma r-\tfrac{\nu}{2}\mathrm{Tr}_{f}X+\tfrac12G(p,p)+\langle Ax+B_{q}x+0_{H},p\rangle_{H}-g(x)=F^{\sharp}(x,r,p,X) γ r − 2 ν Tr f X + 2 1 G ( p , p ) + ⟨ A x + B q x + 0 H , p ⟩ H − g ( x ) = F ♯ ( x , r , p , X ) . Hence F ♯ F^{\sharp} F ♯ is degenerate elliptic by A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §operator , locally strictly proper by A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §proper , and satisfies the second-order structure condition, the tail-insensitivity condition and the shift-continuity condition by A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §structure , A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §tail (with The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §infinite ) and A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §shift : this is clause 3. Since H H H is not finite-dimensional (The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §infinite ), A Viscous Hamilton-Jacobi Operator with a Monotone Nonlinearity Satisfies the Second-Order Comparison Hypotheses §comparison applied to u = w 1 u=w_{1} u = w 1 , v = w 2 v=w_{2} v = w 2 and C C C gives clause 4.
Step 6 (Clause 5: the approximating data). Let w , δ , φ , x ^ w,\delta,\varphi,\hat{x} w , δ , φ , x ^ be as in clause 5; in case (a) put τ = 1 \tau=1 τ = 1 and in case (b) τ = − 1 \tau=-1 τ = − 1 . Since w w w is continuous on H H H , Basic Properties of the δ \delta δ -Envelopes: Semicontinuity, Duality, Closed Superlevel Sets, Bounds and Monotonicity §semicontinuous-case (with U = H U=H U = H , so V ∩ U = V V\cap U=V V ∩ U = V ) shows that w w w is bounded above and below near each point of H H H and that w δ − ( x ) = w ( x ) − δ h ( x ) w^{-}_{\delta}(x)=w(x)-\delta h(x) w δ − ( x ) = w ( x ) − δ h ( x ) and w δ + ( x ) = w ( x ) + δ h ( x ) w^{+}_{\delta}(x)=w(x)+\delta h(x) w δ + ( x ) = w ( x ) + δ h ( x ) for x ∈ V x\in V x ∈ V . Let e e e be w δ − w^{-}_{\delta} w δ − in case (a) and w δ + w^{+}_{\delta} w δ + in case (b); thus e ( x ) = w ( x ) − τ δ h ( x ) e(x)=w(x)-\tau\delta h(x) e ( x ) = w ( x ) − τ δ h ( x ) on V V V , and by hypothesis e − φ e-\varphi e − φ has at x ^ \hat{x} x ^ a local maximum relative to V V V in case (a) and a local minimum relative to V V V in case (b). Put r ^ = w ( x ^ ) − τ δ h ( x ^ ) \hat{r}=w(\hat{x})-\tau\delta h(\hat{x}) r ^ = w ( x ^ ) − τ δ h ( x ^ ) , p ^ = D φ ( x ^ ) ∈ H \hat{p}=D\varphi(\hat{x})\in H p ^ = D φ ( x ^ ) ∈ H and Y ^ = D 2 φ ( x ^ ) ∈ S y m ( H ) \hat{Y}=D^{2}\varphi(\hat{x})\in\mathrm{Sym}(H) Y ^ = D 2 φ ( x ^ ) ∈ Sym ( H ) . For y ∈ H − 1 y\in H^{-1} y ∈ H − 1 , s ∈ R s\in\mathbb{R} s ∈ R , p ∈ H p\in H p ∈ H and Y ∈ S y m ( H ) Y\in\mathrm{Sym}(H) Y ∈ Sym ( H ) let Φ ( y , s , p , Y ) \Phi(y,s,p,Y) Φ ( y , s , p , Y ) be F δ ♯ − ( y , s , p , Y ) F^{\sharp-}_{\delta}(y,s,p,Y) F δ ♯ − ( y , s , p , Y ) in case (a) and F δ ♯ + ( y , s , p , Y ) F^{\sharp+}_{\delta}(y,s,p,Y) F δ ♯ + ( y , s , p , Y ) in case (b); by Second-Order Equation Operator on an Open Subset of a Hilbert Triple and Its δ \delta δ -Shifts §shifted ,
Φ ( y , s , p , Y ) = F ♯ ( y , s + τ δ h ( y ) , p + τ δ A y , Y ∣ V + τ δ I V ) . \Phi(y,s,p,Y)=F^{\sharp}\bigl(y,\ s+\tau\delta h(y),\ p+\tau\delta Ay,\ Y|_{V}+\tau\delta I_{V}\bigr). Φ ( y , s , p , Y ) = F ♯ ( y , s + τ δ h ( y ) , p + τ δ A y , Y ∣ V + τ δ I V ) .
By Viscosity Subsolution, Supersolution and Solution of a Second-Order Equation on a Hilbert Triple §subsolution in case (a), respectively Viscosity Subsolution, Supersolution and Solution of a Second-Order Equation on a Hilbert Triple §supersolution in case (b), applied with U = H U=H U = H , W = D ( A ) = H − 1 W=D(A)=H^{-1} W = D ( A ) = H − 1 , this δ \delta δ , this φ \varphi φ , this x ^ \hat{x} x ^ and ε = 1 / j \varepsilon=1/j ε = 1/ j , we choose for each j ∈ N j\in\mathbb{N} j ∈ N elements y j ∈ H − 1 y_{j}\in H^{-1} y j ∈ H − 1 , s j ∈ R s_{j}\in\mathbb{R} s j ∈ R , p j ∈ H p_{j}\in H p j ∈ H and Y j ∈ S y m ( H ) Y_{j}\in\mathrm{Sym}(H) Y j ∈ Sym ( H ) with
∣ y j − x ^ ∣ H < 1 j , ∣ s j − r ^ ∣ < 1 j , ∣ p j − p ^ ∣ H < 1 j , ∥ Y j − Y ^ ∥ < 1 j , τ Φ ( y j , s j , p j , Y j ) ≤ 1 j |y_{j}-\hat{x}|_{H}<\tfrac1j,\qquad|s_{j}-\hat{r}|<\tfrac1j,\qquad|p_{j}-\hat{p}|_{H}<\tfrac1j,\qquad\lVert Y_{j}-\hat{Y}\rVert<\tfrac1j,\qquad\tau\,\Phi(y_{j},s_{j},p_{j},Y_{j})\le\tfrac1j ∣ y j − x ^ ∣ H < j 1 , ∣ s j − r ^ ∣ < j 1 , ∣ p j − p ^ ∣ H < j 1 , ∥ Y j − Y ^ ∥ < j 1 , τ Φ ( y j , s j , p j , Y j ) ≤ j 1
(in case (b) the last condition is − 1 j ≤ F δ ♯ + ( y j , s j , p j , Y j ) -\tfrac1j\le F^{\sharp+}_{\delta}(y_{j},s_{j},p_{j},Y_{j}) − j 1 ≤ F δ ♯ + ( y j , s j , p j , Y j ) ).
Step 7 (Expansion). Let y ∈ H − 1 y\in H^{-1} y ∈ H − 1 , s ∈ R s\in\mathbb{R} s ∈ R , p ∈ H p\in H p ∈ H , Y ∈ S y m ( H ) Y\in\mathrm{Sym}(H) Y ∈ Sym ( H ) , and put u = p + τ δ A y u=p+\tau\delta Ay u = p + τ δ A y . By The Shifted Hamilton-Jacobi-Bellman Equation of the Wick-Square Problem on the Sobolev Triple of Order Two §operator , Elementary Properties of the Trace of a Form along a Square-Summable Sequence §linear , Elementary Properties of the Trace of a Form along a Square-Summable Sequence §identity and bilinearity of ⟨ ⋅ , ⋅ ⟩ H \langle\cdot,\cdot\rangle_{H} ⟨ ⋅ , ⋅ ⟩ H ,
Φ ( y , s , p , Y ) = Ψ ( y , s , p , Y ) + τ δ ∣ A y ∣ H 2 , \Phi(y,s,p,Y)=\Psi(y,s,p,Y)+\tau\delta|Ay|_{H}^{2}, Φ ( y , s , p , Y ) = Ψ ( y , s , p , Y ) + τ δ ∣ A y ∣ H 2 ,
where
Ψ ( y , s , p , Y ) = γ s + τ γ δ h ( y ) − ν 2 T r f ( Y ∣ V ) − τ ν δ 2 σ ( f ) + 1 2 G ( u , u ) + ⟨ A y , p ⟩ H + ⟨ B q y , p ⟩ H + τ δ ⟨ B q y , A y ⟩ H − g ( y ) . \Psi(y,s,p,Y)=\gamma s+\tau\gamma\delta h(y)-\tfrac{\nu}{2}\mathrm{Tr}_{f}(Y|_{V})-\tfrac{\tau\nu\delta}{2}\sigma(f)+\tfrac12G(u,u)+\langle Ay,p\rangle_{H}+\langle B_{q}y,p\rangle_{H}+\tau\delta\langle B_{q}y,Ay\rangle_{H}-g(y). Ψ ( y , s , p , Y ) = γ s + τ γ δ h ( y ) − 2 ν Tr f ( Y ∣ V ) − 2 τν δ σ ( f ) + 2 1 G ( u , u ) + ⟨ A y , p ⟩ H + ⟨ B q y , p ⟩ H + τ δ ⟨ B q y , A y ⟩ H − g ( y ) .
Step 8 (Coercivity). With y , s , p , Y , u y,s,p,Y,u y , s , p , Y , u as in Step 7, multiply by τ \tau τ (so τ 2 = 1 \tau^{2}=1 τ 2 = 1 ) and bound the terms of τ Ψ \tau\Psi τ Ψ from below: γ δ h ( y ) ≥ 0 \gamma\delta h(y)\ge0 γ δ h ( y ) ≥ 0 ; δ ⟨ B q y , A y ⟩ H ≥ 0 \delta\langle B_{q}y,Ay\rangle_{H}\ge0 δ ⟨ B q y , A y ⟩ H ≥ 0 because B q B_{q} B q is a monotone nonlinearity (The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §drift ), hence A A A -monotone (Monotone, A A A -Monotone and Locally Bounded Nonlinearities on a Hilbert Triple §nonlinearity , Monotone, A A A -Monotone and Locally Bounded Nonlinearities on a Hilbert Triple §a-monotone ); ∣ T r f ( Y ∣ V ) ∣ ≤ ∥ Y ∥ σ ( f ) |\mathrm{Tr}_{f}(Y|_{V})|\le\lVert Y\rVert\sigma(f) ∣ Tr f ( Y ∣ V ) ∣ ≤ ∥ Y ∥ σ ( f ) by Elementary Properties of the Trace of a Form along a Square-Summable Sequence §restriction ; ∣ ⟨ A y , p ⟩ H ∣ ≤ ∣ A y ∣ H ∣ p ∣ H |\langle Ay,p\rangle_{H}|\le|Ay|_{H}|p|_{H} ∣ ⟨ A y , p ⟩ H ∣ ≤ ∣ A y ∣ H ∣ p ∣ H ; ∣ ⟨ B q y , p ⟩ H ∣ ≤ β ∣ y ∣ H ∣ p ∣ H |\langle B_{q}y,p\rangle_{H}|\le\beta|y|_{H}|p|_{H} ∣ ⟨ B q y , p ⟩ H ∣ ≤ β ∣ y ∣ H ∣ p ∣ H by Step 1(a); ∣ g ( y ) ∣ ≤ C g |g(y)|\le C_{g} ∣ g ( y ) ∣ ≤ C g ; and, by Step 1(d) and Step 1(c) with b = A y b=Ay b = A y ,
τ 2 G ( u , u ) ≥ − 1 2 G ( u , u ) ≥ − G ( p , p ) − δ 2 G ( A y , A y ) ≥ − ∣ p ∣ H 2 − δ 2 ∣ y ∣ H ∣ A y ∣ H . \tfrac{\tau}{2}G(u,u)\ge-\tfrac12G(u,u)\ge-G(p,p)-\delta^{2}G(Ay,Ay)\ge-|p|_{H}^{2}-\delta^{2}|y|_{H}\,|Ay|_{H}. 2 τ G ( u , u ) ≥ − 2 1 G ( u , u ) ≥ − G ( p , p ) − δ 2 G ( A y , A y ) ≥ − ∣ p ∣ H 2 − δ 2 ∣ y ∣ H ∣ A y ∣ H .
Since σ ( f ) ≥ 0 \sigma(f)\ge0 σ ( f ) ≥ 0 (Square-Summable Sequences in the Form Space of a Hilbert Triple and the Trace of a Form along Them §square-summable ), with t = ∣ A y ∣ H t=|Ay|_{H} t = ∣ A y ∣ H this gives
τ Φ ( y , s , p , Y ) ≥ δ t 2 − ( ∣ p ∣ H + δ 2 ∣ y ∣ H ) t − ( γ ∣ s ∣ + ν 2 ∥ Y ∥ σ ( f ) + ν δ 2 σ ( f ) + ∣ p ∣ H 2 + β ∣ y ∣ H ∣ p ∣ H + C g ) . \tau\,\Phi(y,s,p,Y)\ge\delta t^{2}-\bigl(|p|_{H}+\delta^{2}|y|_{H}\bigr)t-\Bigl(\gamma|s|+\tfrac{\nu}{2}\lVert Y\rVert\sigma(f)+\tfrac{\nu\delta}{2}\sigma(f)+|p|_{H}^{2}+\beta|y|_{H}|p|_{H}+C_{g}\Bigr). τ Φ ( y , s , p , Y ) ≥ δ t 2 − ( ∣ p ∣ H + δ 2 ∣ y ∣ H ) t − ( γ ∣ s ∣ + 2 ν ∥ Y ∥ σ ( f ) + 2 ν δ σ ( f ) + ∣ p ∣ H 2 + β ∣ y ∣ H ∣ p ∣ H + C g ) .
For the data of Step 6, ∣ y j ∣ H ≤ ∣ x ^ ∣ H + 1 |y_{j}|_{H}\le|\hat{x}|_{H}+1 ∣ y j ∣ H ≤ ∣ x ^ ∣ H + 1 , ∣ s j ∣ ≤ ∣ r ^ ∣ + 1 |s_{j}|\le|\hat{r}|+1 ∣ s j ∣ ≤ ∣ r ^ ∣ + 1 , ∣ p j ∣ H ≤ ∣ p ^ ∣ H + 1 |p_{j}|_{H}\le|\hat{p}|_{H}+1 ∣ p j ∣ H ≤ ∣ p ^ ∣ H + 1 and ∥ Y j ∥ ≤ ∥ Y ^ ∥ + 1 \lVert Y_{j}\rVert\le\lVert\hat{Y}\rVert+1 ∥ Y j ∥ ≤ ∥ Y ^ ∥ + 1 (Elementary Properties of Bounded Symmetric Bilinear Forms: Norm, Quadratic Form, Order and Continuity §norm-axioms ). Put m 0 = ∣ p ^ ∣ H + 1 + δ 2 ( ∣ x ^ ∣ H + 1 ) m_{0}=|\hat{p}|_{H}+1+\delta^{2}(|\hat{x}|_{H}+1) m 0 = ∣ p ^ ∣ H + 1 + δ 2 ( ∣ x ^ ∣ H + 1 ) and K 0 = γ ( ∣ r ^ ∣ + 1 ) + ν 2 ( ∥ Y ^ ∥ + 1 ) σ ( f ) + ν δ 2 σ ( f ) + ( ∣ p ^ ∣ H + 1 ) 2 + β ( ∣ x ^ ∣ H + 1 ) ( ∣ p ^ ∣ H + 1 ) + C g K_{0}=\gamma(|\hat{r}|+1)+\tfrac{\nu}{2}(\lVert\hat{Y}\rVert+1)\sigma(f)+\tfrac{\nu\delta}{2}\sigma(f)+(|\hat{p}|_{H}+1)^{2}+\beta(|\hat{x}|_{H}+1)(|\hat{p}|_{H}+1)+C_{g} K 0 = γ ( ∣ r ^ ∣ + 1 ) + 2 ν (∥ Y ^ ∥ + 1 ) σ ( f ) + 2 ν δ σ ( f ) + ( ∣ p ^ ∣ H + 1 ) 2 + β ( ∣ x ^ ∣ H + 1 ) ( ∣ p ^ ∣ H + 1 ) + C g , and t j = ∣ A y j ∣ H = ∣ y j ∣ H − 1 t_{j}=|Ay_{j}|_{H}=|y_{j}|_{H^{-1}} t j = ∣ A y j ∣ H = ∣ y j ∣ H − 1 . Then δ t j 2 − m 0 t j − K 0 ≤ τ Φ ( y j , s j , p j , Y j ) ≤ 1 \delta t_{j}^{2}-m_{0}t_{j}-K_{0}\le\tau\Phi(y_{j},s_{j},p_{j},Y_{j})\le1 δ t j 2 − m 0 t j − K 0 ≤ τ Φ ( y j , s j , p j , Y j ) ≤ 1 , i.e. δ t j 2 ≤ m 0 t j + K 0 + 1 \delta t_{j}^{2}\le m_{0}t_{j}+K_{0}+1 δ t j 2 ≤ m 0 t j + K 0 + 1 . If t j ≥ 1 t_{j}\ge1 t j ≥ 1 this gives δ t j 2 ≤ ( m 0 + K 0 + 1 ) t j \delta t_{j}^{2}\le(m_{0}+K_{0}+1)t_{j} δ t j 2 ≤ ( m 0 + K 0 + 1 ) t j , so t j ≤ ( m 0 + K 0 + 1 ) / δ t_{j}\le(m_{0}+K_{0}+1)/\delta t j ≤ ( m 0 + K 0 + 1 ) / δ . Hence, with M = max { 1 , ( m 0 + K 0 + 1 ) / δ } M=\max\{1,(m_{0}+K_{0}+1)/\delta\} M = max { 1 , ( m 0 + K 0 + 1 ) / δ } ,
∣ y j ∣ H − 1 ≤ M for every j ∈ N . |y_{j}|_{H^{-1}}\le M\qquad\text{for every }j\in\mathbb{N}. ∣ y j ∣ H − 1 ≤ M for every j ∈ N .
Step 9 (x ^ ∈ H − 1 \hat{x}\in H^{-1} x ^ ∈ H − 1 ). Let k ∈ Z n k\in\mathbb{Z}^{n} k ∈ Z n . By The Sobolev Triple of Order Two for the Wick-Square Problem: the Domain Is the Sobolev Space of Order -1, Unit Families Are Square-Summable, the Gradient Form and the Riccati Drift §pairings and Cauchy-Schwarz in H H H , ∣ y j ( k ) − x ^ ( k ) ∣ = μ k 3 ∣ ⟨ y j − x ^ , e k ⟩ H ∣ ≤ μ k 3 ∣ e k ∣ H / j |y_{j}(k)-\hat{x}(k)|=\mu_{k}^{3}|\langle y_{j}-\hat{x},e_{k}\rangle_{H}|\le\mu_{k}^{3}|e_{k}|_{H}/j ∣ y j ( k ) − x ^ ( k ) ∣ = μ k 3 ∣ ⟨ y j − x ^ , e k ⟩ H ∣ ≤ μ k 3 ∣ e k ∣ H / j , so y j ( k ) → x ^ ( k ) y_{j}(k)\to\hat{x}(k) y j ( k ) → x ^ ( k ) as j → ∞ j\to\infty j → ∞ . Fix N ∈ N N\in\mathbb{N} N ∈ N . By The Wick-Square Problem on the Torus: Standing Notation §state-space and Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §nonnegative , ∑ k ∈ Γ N y j ( k ) 2 / μ k ≤ ∣ y j ∣ H − 1 2 ≤ M 2 \sum_{k\in\Gamma_{N}}y_{j}(k)^{2}/\mu_{k}\le|y_{j}|_{H^{-1}}^{2}\le M^{2} ∑ k ∈ Γ N y j ( k ) 2 / μ k ≤ ∣ y j ∣ H − 1 2 ≤ M 2 for every j j j ; letting j → ∞ j\to\infty j → ∞ in this finite sum gives ∑ k ∈ Γ N x ^ ( k ) 2 / μ k ≤ M 2 \sum_{k\in\Gamma_{N}}\hat{x}(k)^{2}/\mu_{k}\le M^{2} ∑ k ∈ Γ N x ^ ( k ) 2 / μ k ≤ M 2 . By Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §nonnegative , k ↦ x ^ ( k ) 2 / μ k k\mapsto\hat{x}(k)^{2}/\mu_{k} k ↦ x ^ ( k ) 2 / μ k is cube-summable with lattice sum at most M 2 M^{2} M 2 , so by (S) x ^ ∈ H − 1 \hat{x}\in H^{-1} x ^ ∈ H − 1 and ∣ x ^ ∣ H − 1 ≤ M |\hat{x}|_{H^{-1}}\le M ∣ x ^ ∣ H − 1 ≤ M . In particular x ^ ∈ D ( A ) \hat{x}\in D(A) x ^ ∈ D ( A ) and Φ ( x ^ , r ^ , p ^ , Y ^ ) \Phi(\hat{x},\hat{r},\hat{p},\hat{Y}) Φ ( x ^ , r ^ , p ^ , Y ^ ) is defined.
Step 10 (Convergence). Put z j = y j − x ^ ∈ H − 1 z_{j}=y_{j}-\hat{x}\in H^{-1} z j = y j − x ^ ∈ H − 1 , so ∣ z j ∣ H < 1 / j |z_{j}|_{H}<1/j ∣ z j ∣ H < 1/ j , ∣ z j ∣ H − 1 ≤ 2 M |z_{j}|_{H^{-1}}\le2M ∣ z j ∣ H − 1 ≤ 2 M and A z j = A y j − A x ^ Az_{j}=Ay_{j}-A\hat{x} A z j = A y j − A x ^ . (i) By Step 1(b), ∣ z j ∣ V 2 ≤ 2 M / j |z_{j}|_{V}^{2}\le2M/j ∣ z j ∣ V 2 ≤ 2 M / j , so ∣ z j ∣ V → 0 |z_{j}|_{V}\to0 ∣ z j ∣ V → 0 . (ii) Let p ∈ H p\in H p ∈ H and ϵ > 0 \epsilon>0 ϵ > 0 . As V V V is dense in H H H (Hilbert Triples: Standing Notation and Background §triple ), choose v ∈ V v\in V v ∈ V with ∣ p − v ∣ H < ϵ |p-v|_{H}<\epsilon ∣ p − v ∣ H < ϵ ; then by Step 1(b), ∣ ⟨ A z j , p ⟩ H ∣ ≤ ∣ ⟨ z j , v ⟩ V ∣ + ∣ A z j ∣ H ∣ p − v ∣ H ≤ ∣ z j ∣ V ∣ v ∣ V + 2 M ϵ |\langle Az_{j},p\rangle_{H}|\le|\langle z_{j},v\rangle_{V}|+|Az_{j}|_{H}|p-v|_{H}\le|z_{j}|_{V}|v|_{V}+2M\epsilon ∣ ⟨ A z j , p ⟩ H ∣ ≤ ∣ ⟨ z j , v ⟩ V ∣ + ∣ A z j ∣ H ∣ p − v ∣ H ≤ ∣ z j ∣ V ∣ v ∣ V + 2 M ϵ , which by (i) is below ( 1 + 2 M ) ϵ (1+2M)\epsilon ( 1 + 2 M ) ϵ for all large j j j ; so ⟨ A z j , p ⟩ H → 0 \langle Az_{j},p\rangle_{H}\to0 ⟨ A z j , p ⟩ H → 0 . (iii) We show Ψ ( y j , s j , p j , Y j ) → Ψ ( x ^ , r ^ , p ^ , Y ^ ) \Psi(y_{j},s_{j},p_{j},Y_{j})\to\Psi(\hat{x},\hat{r},\hat{p},\hat{Y}) Ψ ( y j , s j , p j , Y j ) → Ψ ( x ^ , r ^ , p ^ , Y ^ ) , term by term. First, s j → r ^ s_{j}\to\hat{r} s j → r ^ ; and ∣ ∣ y j ∣ V − ∣ x ^ ∣ V ∣ ≤ ∣ z j ∣ V → 0 ||y_{j}|_{V}-|\hat{x}|_{V}|\le|z_{j}|_{V}\to0 ∣∣ y j ∣ V − ∣ x ^ ∣ V ∣ ≤ ∣ z j ∣ V → 0 , so h ( y j ) = 1 2 ∣ y j ∣ V 2 → h ( x ^ ) h(y_{j})=\tfrac12|y_{j}|_{V}^{2}\to h(\hat{x}) h ( y j ) = 2 1 ∣ y j ∣ V 2 → h ( x ^ ) ; in particular ( ∣ y j ∣ V ) j (|y_{j}|_{V})_{j} ( ∣ y j ∣ V ) j is bounded, say by M V M_{V} M V . Second, by Elementary Properties of Bounded Symmetric Bilinear Forms: Norm, Quadratic Form, Order and Continuity §restriction , Elementary Properties of the Trace of a Form along a Square-Summable Sequence §linear and Elementary Properties of the Trace of a Form along a Square-Summable Sequence §restriction , ∣ T r f ( Y j ∣ V ) − T r f ( Y ^ ∣ V ) ∣ = ∣ T r f ( ( Y j − Y ^ ) ∣ V ) ∣ ≤ σ ( f ) / j |\mathrm{Tr}_{f}(Y_{j}|_{V})-\mathrm{Tr}_{f}(\hat{Y}|_{V})|=|\mathrm{Tr}_{f}((Y_{j}-\hat{Y})|_{V})|\le\sigma(f)/j ∣ Tr f ( Y j ∣ V ) − Tr f ( Y ^ ∣ V ) ∣ = ∣ Tr f (( Y j − Y ^ ) ∣ V ) ∣ ≤ σ ( f ) / j . Third, with u j = p j + τ δ A y j u_{j}=p_{j}+\tau\delta Ay_{j} u j = p j + τ δ A y j and u ^ = p ^ + τ δ A x ^ \hat{u}=\hat{p}+\tau\delta A\hat{x} u ^ = p ^ + τ δ A x ^ , one has ∣ u j + u ^ ∣ H ≤ 2 ∣ p ^ ∣ H + 1 + 2 δ M |u_{j}+\hat{u}|_{H}\le2|\hat{p}|_{H}+1+2\delta M ∣ u j + u ^ ∣ H ≤ 2∣ p ^ ∣ H + 1 + 2 δ M and u j − u ^ = ( p j − p ^ ) + τ δ A z j u_{j}-\hat{u}=(p_{j}-\hat{p})+\tau\delta Az_{j} u j − u ^ = ( p j − p ^ ) + τ δ A z j , so by Step 1(d) and Step 1(c)
∣ G ( u j , u j ) − G ( u ^ , u ^ ) ∣ = ∣ G ( u j − u ^ , u j + u ^ ) ∣ ≤ ( 1 j + δ ∣ z j ∣ H ) ( 2 ∣ p ^ ∣ H + 1 + 2 δ M ) → 0. |G(u_{j},u_{j})-G(\hat{u},\hat{u})|=|G(u_{j}-\hat{u},u_{j}+\hat{u})|\le\bigl(\tfrac1j+\delta|z_{j}|_{H}\bigr)\bigl(2|\hat{p}|_{H}+1+2\delta M\bigr)\to0. ∣ G ( u j , u j ) − G ( u ^ , u ^ ) ∣ = ∣ G ( u j − u ^ , u j + u ^ ) ∣ ≤ ( j 1 + δ ∣ z j ∣ H ) ( 2∣ p ^ ∣ H + 1 + 2 δ M ) → 0.
Fourth, ⟨ A y j , p j ⟩ H − ⟨ A x ^ , p ^ ⟩ H = ⟨ A z j , p ^ ⟩ H + ⟨ A z j , p j − p ^ ⟩ H + ⟨ A x ^ , p j − p ^ ⟩ H \langle Ay_{j},p_{j}\rangle_{H}-\langle A\hat{x},\hat{p}\rangle_{H}=\langle Az_{j},\hat{p}\rangle_{H}+\langle Az_{j},p_{j}-\hat{p}\rangle_{H}+\langle A\hat{x},p_{j}-\hat{p}\rangle_{H} ⟨ A y j , p j ⟩ H − ⟨ A x ^ , p ^ ⟩ H = ⟨ A z j , p ^ ⟩ H + ⟨ A z j , p j − p ^ ⟩ H + ⟨ A x ^ , p j − p ^ ⟩ H , whose terms tend to 0 0 0 by (ii) and are bounded by 2 M / j 2M/j 2 M / j and M / j M/j M / j . Fifth, by Step 1(a), ∣ ⟨ B q y j , p j ⟩ H − ⟨ B q x ^ , p ^ ⟩ H ∣ ≤ ∣ ⟨ B q z j , p j ⟩ H ∣ + ∣ ⟨ B q x ^ , p j − p ^ ⟩ H ∣ ≤ β ∣ z j ∣ H ( ∣ p ^ ∣ H + 1 ) + β ∣ x ^ ∣ H / j → 0 |\langle B_{q}y_{j},p_{j}\rangle_{H}-\langle B_{q}\hat{x},\hat{p}\rangle_{H}|\le|\langle B_{q}z_{j},p_{j}\rangle_{H}|+|\langle B_{q}\hat{x},p_{j}-\hat{p}\rangle_{H}|\le\beta|z_{j}|_{H}(|\hat{p}|_{H}+1)+\beta|\hat{x}|_{H}/j\to0 ∣ ⟨ B q y j , p j ⟩ H − ⟨ B q x ^ , p ^ ⟩ H ∣ ≤ ∣ ⟨ B q z j , p j ⟩ H ∣ + ∣ ⟨ B q x ^ , p j − p ^ ⟩ H ∣ ≤ β ∣ z j ∣ H ( ∣ p ^ ∣ H + 1 ) + β ∣ x ^ ∣ H / j → 0 . Sixth, by Step 1(a) (B q z j , B q x ^ ∈ V B_{q}z_{j},B_{q}\hat{x}\in V B q z j , B q x ^ ∈ V ) and Step 1(b),
⟨ B q y j , A y j ⟩ H − ⟨ B q x ^ , A x ^ ⟩ H = ⟨ A y j , B q z j ⟩ H + ⟨ A z j , B q x ^ ⟩ H = ⟨ y j , B q z j ⟩ V + ⟨ z j , B q x ^ ⟩ V , \langle B_{q}y_{j},Ay_{j}\rangle_{H}-\langle B_{q}\hat{x},A\hat{x}\rangle_{H}=\langle Ay_{j},B_{q}z_{j}\rangle_{H}+\langle Az_{j},B_{q}\hat{x}\rangle_{H}=\langle y_{j},B_{q}z_{j}\rangle_{V}+\langle z_{j},B_{q}\hat{x}\rangle_{V}, ⟨ B q y j , A y j ⟩ H − ⟨ B q x ^ , A x ^ ⟩ H = ⟨ A y j , B q z j ⟩ H + ⟨ A z j , B q x ^ ⟩ H = ⟨ y j , B q z j ⟩ V + ⟨ z j , B q x ^ ⟩ V ,
of absolute value at most β M V ∣ z j ∣ V + β ∣ x ^ ∣ V ∣ z j ∣ V → 0 \beta M_{V}|z_{j}|_{V}+\beta|\hat{x}|_{V}|z_{j}|_{V}\to0 β M V ∣ z j ∣ V + β ∣ x ^ ∣ V ∣ z j ∣ V → 0 by (i). Seventh, ∣ g ( y j ) − g ( x ^ ) ∣ ≤ ℓ g / j |g(y_{j})-g(\hat{x})|\le\ell_{g}/j ∣ g ( y j ) − g ( x ^ ) ∣ ≤ ℓ g / j . By the limit laws, Ψ ( y j , s j , p j , Y j ) → Ψ ( x ^ , r ^ , p ^ , Y ^ ) \Psi(y_{j},s_{j},p_{j},Y_{j})\to\Psi(\hat{x},\hat{r},\hat{p},\hat{Y}) Ψ ( y j , s j , p j , Y j ) → Ψ ( x ^ , r ^ , p ^ , Y ^ ) .
Step 11 (Conclusion of clause 5). Since A y j = A x ^ + A z j Ay_{j}=A\hat{x}+Az_{j} A y j = A x ^ + A z j , ∣ A y j ∣ H 2 = ∣ A x ^ ∣ H 2 + 2 ⟨ A z j , A x ^ ⟩ H + ∣ A z j ∣ H 2 ≥ ∣ A x ^ ∣ H 2 + 2 ⟨ A z j , A x ^ ⟩ H |Ay_{j}|_{H}^{2}=|A\hat{x}|_{H}^{2}+2\langle Az_{j},A\hat{x}\rangle_{H}+|Az_{j}|_{H}^{2}\ge|A\hat{x}|_{H}^{2}+2\langle Az_{j},A\hat{x}\rangle_{H} ∣ A y j ∣ H 2 = ∣ A x ^ ∣ H 2 + 2 ⟨ A z j , A x ^ ⟩ H + ∣ A z j ∣ H 2 ≥ ∣ A x ^ ∣ H 2 + 2 ⟨ A z j , A x ^ ⟩ H . By Steps 6 and 7,
1 j ≥ τ Φ ( y j , s j , p j , Y j ) = τ Ψ ( y j , s j , p j , Y j ) + δ ∣ A y j ∣ H 2 ≥ τ Ψ ( y j , s j , p j , Y j ) + δ ∣ A x ^ ∣ H 2 + 2 δ ⟨ A z j , A x ^ ⟩ H . \tfrac1j\ge\tau\,\Phi(y_{j},s_{j},p_{j},Y_{j})=\tau\,\Psi(y_{j},s_{j},p_{j},Y_{j})+\delta|Ay_{j}|_{H}^{2}\ge\tau\,\Psi(y_{j},s_{j},p_{j},Y_{j})+\delta|A\hat{x}|_{H}^{2}+2\delta\langle Az_{j},A\hat{x}\rangle_{H}. j 1 ≥ τ Φ ( y j , s j , p j , Y j ) = τ Ψ ( y j , s j , p j , Y j ) + δ ∣ A y j ∣ H 2 ≥ τ Ψ ( y j , s j , p j , Y j ) + δ ∣ A x ^ ∣ H 2 + 2 δ ⟨ A z j , A x ^ ⟩ H .
By Step 10(iii) and Step 10(ii) with p = A x ^ p=A\hat{x} p = A x ^ , the right-hand side converges to τ Ψ ( x ^ , r ^ , p ^ , Y ^ ) + δ ∣ A x ^ ∣ H 2 = τ Φ ( x ^ , r ^ , p ^ , Y ^ ) \tau\Psi(\hat{x},\hat{r},\hat{p},\hat{Y})+\delta|A\hat{x}|_{H}^{2}=\tau\Phi(\hat{x},\hat{r},\hat{p},\hat{Y}) τ Ψ ( x ^ , r ^ , p ^ , Y ^ ) + δ ∣ A x ^ ∣ H 2 = τ Φ ( x ^ , r ^ , p ^ , Y ^ ) (Step 7), and the left-hand side to 0 0 0 ; by the order of limits, τ Φ ( x ^ , r ^ , p ^ , Y ^ ) ≤ 0 \tau\Phi(\hat{x},\hat{r},\hat{p},\hat{Y})\le0 τ Φ ( x ^ , r ^ , p ^ , Y ^ ) ≤ 0 . Together with x ^ ∈ H − 1 \hat{x}\in H^{-1} x ^ ∈ H − 1 (Step 9), in case (a), where τ = 1 \tau=1 τ = 1 and r ^ = w ( x ^ ) − δ h ( x ^ ) \hat{r}=w(\hat{x})-\delta h(\hat{x}) r ^ = w ( x ^ ) − δ h ( x ^ ) , this is F δ ♯ − ( x ^ , w ( x ^ ) − δ h ( x ^ ) , D φ ( x ^ ) , D 2 φ ( x ^ ) ) ≤ 0 F^{\sharp-}_{\delta}(\hat{x},w(\hat{x})-\delta h(\hat{x}),D\varphi(\hat{x}),D^{2}\varphi(\hat{x}))\le0 F δ ♯ − ( x ^ , w ( x ^ ) − δ h ( x ^ ) , D φ ( x ^ ) , D 2 φ ( x ^ )) ≤ 0 ; in case (b), where τ = − 1 \tau=-1 τ = − 1 and r ^ = w ( x ^ ) + δ h ( x ^ ) \hat{r}=w(\hat{x})+\delta h(\hat{x}) r ^ = w ( x ^ ) + δ h ( x ^ ) , it is 0 ≤ F δ ♯ + ( x ^ , w ( x ^ ) + δ h ( x ^ ) , D φ ( x ^ ) , D 2 φ ( x ^ ) ) 0\le F^{\sharp+}_{\delta}(\hat{x},w(\hat{x})+\delta h(\hat{x}),D\varphi(\hat{x}),D^{2}\varphi(\hat{x})) 0 ≤ F δ ♯ + ( x ^ , w ( x ^ ) + δ h ( x ^ ) , D φ ( x ^ ) , D 2 φ ( x ^ )) . This proves clause 5 and completes the proof.