Each result cited is universally quantified over the data in its own statement.
Throughout, ψ k \psi_{k} ψ k , μ k \mu_{k} μ k , λ Q \lambda_{Q} λ Q , a j − 1 / 2 = 1 / a j 1 / 2 a_{j}^{-1/2}=1/a_{j}^{1/2} a j − 1/2 = 1/ a j 1/2 , x ( k ) x(k) x ( k ) , Γ L \Gamma_{L} Γ L , d L d_{L} d L , J L J_{L} J L , Φ L [ x ] \Phi_{L}[x] Φ L [ x ] , C L C_{L} C L and f L f_{L} f L (L ∈ N L\in\mathbb{N} L ∈ N ) are as in The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus , x j = ⟨ x , e j ⟩ x_{j}=\langle x,e_{j}\rangle x j = ⟨ x , e j ⟩ , E [ F ] \mathbb{E}[F] E [ F ] denotes ∫ X F d γ c \int_{X}F\,d\gamma_{c} ∫ X F d γ c , and d z dz d z stands for λ Q ( d z ) \lambda_{Q}(dz) λ Q ( d z ) . Put b 4 = ϰ / 4 b_{4}=\varkappa/4 b 4 = ϰ /4 , b 2 = m / 2 b_{2}=\mathfrak{m}/2 b 2 = m /2 and f L ♯ ( s ) = ϰ ( s 3 − 3 C L s ) + m s f^{\sharp}_{L}(s)=\varkappa(s^{3}-3C_{L}s)+\mathfrak{m}s f L ♯ ( s ) = ϰ ( s 3 − 3 C L s ) + m s . By Hermite Polynomials: Low Orders, Derivatives, Recursion, Scaling, the Addition Formula, Gaussian Orthogonality and the Mehler Identity §low-orders and The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §polynomial ,
f L = b 4 H 4 C L + b 2 H 2 C L , f L ♯ = ϰ H 3 C L + m H 1 C L . f_{L}=b_{4}H^{C_{L}}_{4}+b_{2}H^{C_{L}}_{2},\qquad f^{\sharp}_{L}=\varkappa H^{C_{L}}_{3}+\mathfrak{m}H^{C_{L}}_{1}. f L = b 4 H 4 C L + b 2 H 2 C L , f L ♯ = ϰ H 3 C L + m H 1 C L .
Fix N , M ∈ N N,M\in\mathbb{N} N , M ∈ N with N ≤ M N\le M N ≤ M , and let L , L ′ L,L' L , L ′ range over { N , M } \{N,M\} { N , M } , L ∧ L ′ L\wedge L' L ∧ L ′ being the smaller one.
Step 0 (Indices, and a finite interchange rule). By The Cubes of the Integer Lattice are Finite, Nested, Exhaust the Lattice and Have (2N+1)^n Points §nested , Γ N ⊆ Γ M \Gamma_{N}\subseteq\Gamma_{M} Γ N ⊆ Γ M ; as κ ( d N ) ∈ Γ N ⊆ Γ M \kappa(d_{N})\in\Gamma_{N}\subseteq\Gamma_{M} κ ( d N ) ∈ Γ N ⊆ Γ M and d M d_{M} d M is the largest j j j with κ ( j ) ∈ Γ M \kappa(j)\in\Gamma_{M} κ ( j ) ∈ Γ M (The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §head-dimension ), d N ≤ d M d_{N}\le d_{M} d N ≤ d M and J N ⊆ J M J_{N}\subseteq J_{M} J N ⊆ J M . Every j j j with κ ( j ) ∈ Γ L \kappa(j)\in\Gamma_{L} κ ( j ) ∈ Γ L satisfies j ≤ d L j\le d_{L} j ≤ d L , so κ \kappa κ maps J L J_{L} J L bijectively onto Γ L \Gamma_{L} Γ L ; J N ≠ ∅ J_{N}\neq\emptyset J N = ∅ since the zero point lies in Γ N \Gamma_{N} Γ N (The Cubes of the Integer Lattice are Finite, Nested, Exhaust the Lattice and Have (2N+1)^n Points §finite ). Put J N , M = J M ∖ J N J_{N,M}=J_{M}\setminus J_{N} J N , M = J M ∖ J N . A sum ∑ j ∈ I u j \sum_{j\in I}u_{j} ∑ j ∈ I u j over a subset I I I of [ d M ] [d_{M}] [ d M ] , such as J L J_{L} J L or J N , M J_{N,M} J N , M , means the finite sum ∑ j = 1 d M 1 I ( j ) u j \sum_{j=1}^{d_{M}}\mathbf{1}_{I}(j)\,u_{j} ∑ j = 1 d M 1 I ( j ) u j ; in particular it is 0 0 0 if I = ∅ I=\emptyset I = ∅ . By The Galerkin Wick-Ordered Phi^4 Potential on the Torus is an Admissible Cylindrical Potential, with Semiconvexity Constant the Positive Part of Three Times the Coupling Times the Wick Constant Minus the Mass §noise-norm , x ( κ ( j ) ) = a j − 1 / 2 x j x(\kappa(j))=a_{j}^{-1/2}x_{j} x ( κ ( j )) = a j − 1/2 x j for j ∈ [ d L ] j\in[d_{L}] j ∈ [ d L ] , so by The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §field
Φ L [ x ] ( z ) = ∑ j ∈ J L a j − 1 / 2 x j ψ κ ( j ) ( z ) , Φ M [ x ] ( z ) = Φ N [ x ] ( z ) + Ψ [ x ] ( z ) , Ψ [ x ] ( z ) = ∑ j ∈ J N , M a j − 1 / 2 x j ψ κ ( j ) ( z ) (0.1) \Phi_{L}[x](z)=\sum_{j\in J_{L}}a_{j}^{-1/2}x_{j}\psi_{\kappa(j)}(z),\qquad \Phi_{M}[x](z)=\Phi_{N}[x](z)+\Psi[x](z),\quad \Psi[x](z)=\sum_{j\in J_{N,M}}a_{j}^{-1/2}x_{j}\psi_{\kappa(j)}(z)\tag{0.1} Φ L [ x ] ( z ) = j ∈ J L ∑ a j − 1/2 x j ψ κ ( j ) ( z ) , Φ M [ x ] ( z ) = Φ N [ x ] ( z ) + Ψ [ x ] ( z ) , Ψ [ x ] ( z ) = j ∈ J N , M ∑ a j − 1/2 x j ψ κ ( j ) ( z ) ( 0.1 )
(Ψ = 0 \Psi=0 Ψ = 0 if J N , M = ∅ J_{N,M}=\emptyset J N , M = ∅ ). Call F : X × ( R n ) q → R F:X\times(\mathbb{R}^{n})^{q}\to\mathbb{R} F : X × ( R n ) q → R (q ∈ { 1 , 2 } q\in\{1,2\} q ∈ { 1 , 2 } ) elementary if F ( x , y ) = ∑ t = 1 ν g t ( y ) m t ( x ) F(x,y)=\sum_{t=1}^{\nu}g_{t}(y)m_{t}(x) F ( x , y ) = ∑ t = 1 ν g t ( y ) m t ( x ) for some ν ∈ N \nu\in\mathbb{N} ν ∈ N , each g t g_{t} g t a finite product of maps y ↦ ψ k ( y i ) y\mapsto\psi_{k}(y_{i}) y ↦ ψ k ( y i ) and each m t m_{t} m t a real multiple of a finite product of coordinate maps x ↦ x j x\mapsto x_{j} x ↦ x j (empty products being 1 1 1 ). By (0.1) and expansion of finite products, every polynomial with constant coefficients in finitely many of the quantities Φ L [ x ] ( z ) \Phi_{L}[x](z) Φ L [ x ] ( z ) , Ψ [ x ] ( z ) \Psi[x](z) Ψ [ x ] ( z ) , Φ L [ x ] ( w ) \Phi_{L}[x](w) Φ L [ x ] ( w ) , ψ k ( z ) \psi_{k}(z) ψ k ( z ) , ψ k ( w ) \psi_{k}(w) ψ k ( w ) is elementary. For elementary F F F : each m t m_{t} m t is a finite linear combination of functions H β H_{\beta} H β by Cylindrical Hermite Polynomials: Growth and Integrability, Partial Derivatives, Orthogonality, and Monomials as Hermite Combinations §monomials , each Borel and in L p ( γ c ) L^{p}(\gamma_{c}) L p ( γ c ) for all p ≥ 1 p\ge1 p ≥ 1 by Cylindrical Hermite Polynomials: Growth and Integrability, Partial Derivatives, Orthogonality, and Monomials as Hermite Combinations §cylindrical ; so m t m_{t} m t and 1 A m t \mathbf{1}_{A}m_{t} 1 A m t (A A A Borel) are Borel and γ c \gamma_{c} γ c -integrable. Each finite product of maps ψ k \psi_{k} ψ k lies in C p e r C_{\mathrm{per}} C per by Elementary Properties of Lattice-Periodic Functions §algebra , so its restriction to Q Q Q is λ Q \lambda_{Q} λ Q -integrable by Continuous Periodic Functions are Power-Integrable and Dense on the Torus §member . For q = 1 q=1 q = 1 , ∫ Q F ( x , z ) d z = ∑ t ( ∫ Q g t ) m t ( x ) \int_{Q}F(x,z)\,dz=\sum_{t}(\int_{Q}g_{t})m_{t}(x) ∫ Q F ( x , z ) d z = ∑ t ( ∫ Q g t ) m t ( x ) , and linearity of both integrals gives, for Borel A ⊆ X A\subseteq X A ⊆ X ,
E [ 1 A ∫ Q F ( ⋅ , z ) d z ] = ∑ t ( ∫ Q g t ) E [ 1 A m t ] = ∫ Q E [ 1 A F ( ⋅ , z ) ] d z . (0.2) \mathbb{E}\Bigl[\mathbf{1}_{A}\int_{Q}F(\cdot,z)\,dz\Bigr]=\sum_{t}\Bigl(\int_{Q}g_{t}\Bigr)\mathbb{E}[\mathbf{1}_{A}m_{t}]=\int_{Q}\mathbb{E}[\mathbf{1}_{A}F(\cdot,z)]\,dz.\tag{0.2} E [ 1 A ∫ Q F ( ⋅ , z ) d z ] = t ∑ ( ∫ Q g t ) E [ 1 A m t ] = ∫ Q E [ 1 A F ( ⋅ , z )] d z . ( 0.2 )
For q = 2 q=2 q = 2 each g t ( z , w ) = α t ( z ) β t ( w ) g_{t}(z,w)=\alpha_{t}(z)\beta_{t}(w) g t ( z , w ) = α t ( z ) β t ( w ) with α t , β t \alpha_{t},\beta_{t} α t , β t finite products of maps ψ k \psi_{k} ψ k , and the same computation gives
E [ ∫ Q ( ∫ Q F ( ⋅ , z , w ) d w ) d z ] = ∫ Q ( ∫ Q E [ F ( ⋅ , z , w ) ] d w ) d z . (0.3) \mathbb{E}\Bigl[\int_{Q}\Bigl(\int_{Q}F(\cdot,z,w)\,dw\Bigr)dz\Bigr]=\int_{Q}\Bigl(\int_{Q}\mathbb{E}[F(\cdot,z,w)]\,dw\Bigr)dz.\tag{0.3} E [ ∫ Q ( ∫ Q F ( ⋅ , z , w ) d w ) d z ] = ∫ Q ( ∫ Q E [ F ( ⋅ , z , w )] d w ) d z . ( 0.3 )
Step 1 (Wick-power form). For z ∈ R n z\in\mathbb{R}^{n} z ∈ R n put
h z L = ∑ j ∈ J L c j a j − 1 / 2 ψ κ ( j ) ( z ) e j , g z = ∑ j ∈ J N , M c j a j − 1 / 2 ψ κ ( j ) ( z ) e j . h^{L}_{z}=\sum_{j\in J_{L}}c_{j}a_{j}^{-1/2}\psi_{\kappa(j)}(z)\,e_{j},\qquad g_{z}=\sum_{j\in J_{N,M}}c_{j}a_{j}^{-1/2}\psi_{\kappa(j)}(z)\,e_{j}. h z L = j ∈ J L ∑ c j a j − 1/2 ψ κ ( j ) ( z ) e j , g z = j ∈ J N , M ∑ c j a j − 1/2 ψ κ ( j ) ( z ) e j .
By orthonormality of ( e j ) (e_{j}) ( e j ) (White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §basis ) their coordinates vanish beyond d M d_{M} d M , so the series of The Cameron-Martin Space of a Diagonal Gaussian Measure on a Hilbert Space §space has finitely many nonzero terms and h z L , g z ∈ H c h^{L}_{z},g_{z}\in H_{c} h z L , g z ∈ H c ; the partial sums of The Paley-Wiener Functional of a Vector Relative to a Variance Sequence §partial-sums are constant from d M d_{M} d M on, so by The Paley-Wiener Functional of a Vector Relative to a Variance Sequence §functional and (0.1), ℓ h z L ( x ) = Φ L [ x ] ( z ) \ell_{h^{L}_{z}}(x)=\Phi_{L}[x](z) ℓ h z L ( x ) = Φ L [ x ] ( z ) and ℓ g z ( x ) = Ψ [ x ] ( z ) \ell_{g_{z}}(x)=\Psi[x](z) ℓ g z ( x ) = Ψ [ x ] ( z ) . Since c j ( a j − 1 / 2 ) 2 = c j / a j = μ κ ( j ) − 1 c_{j}(a_{j}^{-1/2})^{2}=c_{j}/a_{j}=\mu_{\kappa(j)}^{-1} c j ( a j − 1/2 ) 2 = c j / a j = μ κ ( j ) − 1 by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §ratio , The Cameron-Martin Inner Product of Two Cameron-Martin Vectors §inner-product , The Cameron-Martin Space of a Diagonal Gaussian Measure on a Hilbert Space §square , J N ⊆ J M J_{N}\subseteq J_{M} J N ⊆ J M and Step 0 give
⟨ h z L , h w L ′ ⟩ c = K L ∧ L ′ ( z , w ) , K L ( z , w ) : = ∑ j ∈ J L μ κ ( j ) − 1 ψ κ ( j ) ( z ) ψ κ ( j ) ( w ) = ∑ k ∈ Γ L μ k − 1 ψ k ( z ) ψ k ( w ) , \langle h^{L}_{z},h^{L'}_{w}\rangle_{c}=\mathcal{K}_{L\wedge L'}(z,w),\qquad \mathcal{K}_{L}(z,w):=\sum_{j\in J_{L}}\mu_{\kappa(j)}^{-1}\psi_{\kappa(j)}(z)\psi_{\kappa(j)}(w)=\sum_{k\in\Gamma_{L}}\mu_{k}^{-1}\psi_{k}(z)\psi_{k}(w), ⟨ h z L , h w L ′ ⟩ c = K L ∧ L ′ ( z , w ) , K L ( z , w ) := j ∈ J L ∑ μ κ ( j ) − 1 ψ κ ( j ) ( z ) ψ κ ( j ) ( w ) = k ∈ Γ L ∑ μ k − 1 ψ k ( z ) ψ k ( w ) ,
and, by The Galerkin Wick-Ordered Phi^4 Potential on the Torus is an Admissible Cylindrical Potential, with Semiconvexity Constant the Positive Part of Three Times the Coupling Times the Wick Constant Minus the Mass §wick , ∣ h z L ∣ c 2 = K L ( z , z ) = C L |h^{L}_{z}|_{c}^{2}=\mathcal{K}_{L}(z,z)=C_{L} ∣ h z L ∣ c 2 = K L ( z , z ) = C L and ∣ g z ∣ c 2 = K M ( z , z ) − K N ( z , z ) = C M − C N = : ϑ ≥ 0 |g_{z}|_{c}^{2}=\mathcal{K}_{M}(z,z)-\mathcal{K}_{N}(z,z)=C_{M}-C_{N}=:\vartheta\ge0 ∣ g z ∣ c 2 = K M ( z , z ) − K N ( z , z ) = C M − C N =: ϑ ≥ 0 . Hence, by The Wick Powers of a Paley-Wiener Functional §wick ,
f L ( Φ L [ x ] ( z ) ) = b 4 : ℓ h z L 4 : ( x ) + b 2 : ℓ h z L 2 : ( x ) , f L ♯ ( Φ L [ x ] ( z ) ) = ϰ : ℓ h z L 3 : ( x ) + m : ℓ h z L 1 : ( x ) , H r ϑ ( Ψ [ x ] ( z ) ) = : ℓ g z r : ( x ) . (1.1) f_{L}(\Phi_{L}[x](z))=b_{4}{:}\ell_{h^{L}_{z}}^{4}{:}(x)+b_{2}{:}\ell_{h^{L}_{z}}^{2}{:}(x),\quad f^{\sharp}_{L}(\Phi_{L}[x](z))=\varkappa{:}\ell_{h^{L}_{z}}^{3}{:}(x)+\mathfrak{m}{:}\ell_{h^{L}_{z}}^{1}{:}(x),\quad H^{\vartheta}_{r}(\Psi[x](z))={:}\ell_{g_{z}}^{r}{:}(x).\tag{1.1} f L ( Φ L [ x ] ( z )) = b 4 : ℓ h z L 4 : ( x ) + b 2 : ℓ h z L 2 : ( x ) , f L ♯ ( Φ L [ x ] ( z )) = ϰ : ℓ h z L 3 : ( x ) + m : ℓ h z L 1 : ( x ) , H r ϑ ( Ψ [ x ] ( z )) = : ℓ g z r : ( x ) . ( 1.1 )
Step 2 (The derivatives). For k ∈ Z n k\in\mathbb{Z}^{n} k ∈ Z n put D k L ( x ) = ∫ Q f L ♯ ( Φ L [ x ] ( z ) ) ψ k ( z ) d z D^{L}_{k}(x)=\int_{Q}f^{\sharp}_{L}(\Phi_{L}[x](z))\psi_{k}(z)\,dz D k L ( x ) = ∫ Q f L ♯ ( Φ L [ x ] ( z )) ψ k ( z ) d z . We claim ∂ j V L = a j − 1 / 2 D κ ( j ) L \partial_{j}V_{L}=a_{j}^{-1/2}D^{L}_{\kappa(j)} ∂ j V L = a j − 1/2 D κ ( j ) L for j ∈ J L j\in J_{L} j ∈ J L and ∂ j V L = 0 \partial_{j}V_{L}=0 ∂ j V L = 0 for j ∈ N ∖ J L j\in\mathbb{N}\setminus J_{L} j ∈ N ∖ J L . By Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient , ∂ j V L = 0 \partial_{j}V_{L}=0 ∂ j V L = 0 for j > d L j>d_{L} j > d L , ∂ j V L ( x ) = ∂ j v L ( p d L ( x ) ) \partial_{j}V_{L}(x)=\partial_{j}v_{L}(p_{d_{L}}(x)) ∂ j V L ( x ) = ∂ j v L ( p d L ( x )) for j ≤ d L j\le d_{L} j ≤ d L , which vanishes for j ∈ [ d L ] ∖ J L j\in[d_{L}]\setminus J_{L} j ∈ [ d L ] ∖ J L by The Galerkin Wick-Ordered Phi^4 Potential on the Torus is an Admissible Cylindrical Potential, with Semiconvexity Constant the Positive Part of Three Times the Coupling Times the Wick Constant Minus the Mass §hessian , and ∇ a V L ( x ) = ∑ j = 1 d L a j ∂ j V L ( x ) e j \nabla_{a}V_{L}(x)=\sum_{j=1}^{d_{L}}a_{j}\partial_{j}V_{L}(x)e_{j} ∇ a V L ( x ) = ∑ j = 1 d L a j ∂ j V L ( x ) e j . By The Galerkin Wick-Ordered Phi^4 Potential on the Torus is an Admissible Cylindrical Potential, with Semiconvexity Constant the Positive Part of Three Times the Coupling Times the Wick Constant Minus the Mass §gradient and E ^ κ ( j ) = a j 1 / 2 e j \hat{E}_{\kappa(j)}=a_{j}^{1/2}e_{j} E ^ κ ( j ) = a j 1/2 e j (White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §basis-vectors ), ∇ a V L ( x ) = ∑ j ∈ J L a j 1 / 2 D κ ( j ) L ( x ) e j \nabla_{a}V_{L}(x)=\sum_{j\in J_{L}}a_{j}^{1/2}D^{L}_{\kappa(j)}(x)e_{j} ∇ a V L ( x ) = ∑ j ∈ J L a j 1/2 D κ ( j ) L ( x ) e j . Pairing with e j e_{j} e j (j ∈ J L j\in J_{L} j ∈ J L ) gives a j ∂ j V L ( x ) = a j 1 / 2 D κ ( j ) L ( x ) a_{j}\partial_{j}V_{L}(x)=a_{j}^{1/2}D^{L}_{\kappa(j)}(x) a j ∂ j V L ( x ) = a j 1/2 D κ ( j ) L ( x ) , and a j > 0 a_{j}>0 a j > 0 .
Step 3 (Claim 1). Take L = N L=N L = N . Expanding the polynomial f N f_{N} f N of degree 4 4 4 in (0.1), f N ( Φ N [ x ] ( z ) ) = ∑ t g t ( z ) m t ( x ) f_{N}(\Phi_{N}[x](z))=\sum_{t}g_{t}(z)m_{t}(x) f N ( Φ N [ x ] ( z )) = ∑ t g t ( z ) m t ( x ) is elementary with each m t m_{t} m t a multiple of ∏ s = 1 r x j s = ∏ k = 1 d N x k α k \prod_{s=1}^{r}x_{j_{s}}=\prod_{k=1}^{d_{N}}x_{k}^{\alpha_{k}} ∏ s = 1 r x j s = ∏ k = 1 d N x k α k , r ≤ 4 r\le4 r ≤ 4 , j s ∈ J N j_{s}\in J_{N} j s ∈ J N , ∣ α ∣ = r |\alpha|=r ∣ α ∣ = r . So V N = ∑ t ( ∫ Q g t ) m t V_{N}=\sum_{t}(\int_{Q}g_{t})m_{t} V N = ∑ t ( ∫ Q g t ) m t (The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §potential ) is, by Cylindrical Hermite Polynomials: Growth and Integrability, Partial Derivatives, Orthogonality, and Monomials as Hermite Combinations §monomials , a finite linear combination of functions H β H_{\beta} H β with ∣ β ∣ ≤ 4 |\beta|\le4 ∣ β ∣ ≤ 4 ; these are Borel and square-integrable by Cylindrical Hermite Polynomials: Growth and Integrability, Partial Derivatives, Orthogonality, and Monomials as Hermite Combinations §cylindrical , so V N V_{N} V N is square-integrable and its class lies in the span of { H β : ∣ β ∣ ≤ 4 } \{H_{\beta}:|\beta|\le4\} { H β : ∣ β ∣ ≤ 4 } , contained in H ≤ 4 \mathcal{H}_{\le4} H ≤ 4 (The Wiener Chaoses of a Diagonal Gaussian Measure on a Hilbert Space §chaos-up-to ). For j ∈ J N j\in J_{N} j ∈ J N , Step 2 and the same argument with f N ♯ f^{\sharp}_{N} f N ♯ of degree 3 3 3 give the assertion for ∂ j V N \partial_{j}V_{N} ∂ j V N with H ≤ 3 \mathcal{H}_{\le3} H ≤ 3 ; for j ∉ J N j\notin J_{N} j ∈ / J N , ∂ j V N = 0 \partial_{j}V_{N}=0 ∂ j V N = 0 , whose class is the zero vector of H ≤ 3 \mathcal{H}_{\le3} H ≤ 3 . As N N N was arbitrary, claim 1 holds.
Step 4 (Independence of coordinate blocks). Let d ∈ N d\in\mathbb{N} d ∈ N , let I 1 , I 2 ⊆ [ d ] I_{1},I_{2}\subseteq[d] I 1 , I 2 ⊆ [ d ] be disjoint and nonempty, and let G i \mathcal{G}_{i} G i be the σ \sigma σ -algebra generated by the maps x ↦ x j x\mapsto x_{j} x ↦ x j , j ∈ I i j\in I_{i} j ∈ I i . We show γ c ( A 1 ∩ A 2 ) = γ c ( A 1 ) γ c ( A 2 ) \gamma_{c}(A_{1}\cap A_{2})=\gamma_{c}(A_{1})\gamma_{c}(A_{2}) γ c ( A 1 ∩ A 2 ) = γ c ( A 1 ) γ c ( A 2 ) for A i ∈ G i A_{i}\in\mathcal{G}_{i} A i ∈ G i , so that G 1 , G 2 \mathcal{G}_{1},\mathcal{G}_{2} G 1 , G 2 are independent (Sigma-Algebra Generated by Random Variables and Independence of Sigma-Algebras ). Write I i = { j 1 < ⋯ < j p } I_{i}=\{j_{1}<\dots<j_{p}\} I i = { j 1 < ⋯ < j p } (p = p i p=p_{i} p = p i ), π i ( x ) = ( x j 1 , … , x j p ) \pi_{i}(x)=(x_{j_{1}},\dots,x_{j_{p}}) π i ( x ) = ( x j 1 , … , x j p ) , and let B p \mathcal{B}_{p} B p be the product Borel σ \sigma σ -algebra of Joint Distribution, Expectations, and Block Independence for Independent Random Variables . The sets π i − 1 ( D ) \pi_{i}^{-1}(D) π i − 1 ( D ) , D ∈ B p D\in\mathcal{B}_{p} D ∈ B p , form a σ \sigma σ -algebra (preimages commute with complements and countable unions) containing each x j l − 1 ( B ) x_{j_{l}}^{-1}(B) x j l − 1 ( B ) , B B B Borel, which is π i − 1 \pi_{i}^{-1} π i − 1 of the preimage of B B B under the l l l -th coordinate projection, jointly Borel by claim 4 of Joint Distribution, Expectations, and Block Independence for Independent Random Variables . Hence A i = π i − 1 ( D i ) A_{i}=\pi_{i}^{-1}(D_{i}) A i = π i − 1 ( D i ) with D i ∈ B p i D_{i}\in\mathcal{B}_{p_{i}} D i ∈ B p i . By Existence of Independent and Identically Distributed Sequences there is a probability space ( Ω , F , P ) (\Omega,\mathcal{F},P) ( Ω , F , P ) with an independent sequence ( ξ k ) (\xi_{k}) ( ξ k ) of standard normal random variables; with Y Y Y and G G G as in The Diagonal Gaussian Random Series in a Hilbert Space: Almost Sure Convergence, Finite-Dimensional Projections, and the Unique Measure with Diagonal Gaussian Projections , claim The Diagonal Gaussian Random Series in a Hilbert Space: Almost Sure Convergence, Finite-Dimensional Projections, and the Unique Measure with Diagonal Gaussian Projections §unique and Diagonal Gaussian Measures on a Hilbert Space §measure give γ c = P Y \gamma_{c}=P_{Y} γ c = P Y , The Diagonal Gaussian Random Series in a Hilbert Space: Almost Sure Convergence, Finite-Dimensional Projections, and the Unique Measure with Diagonal Gaussian Projections §convergence gives P ( G ) = 1 P(G)=1 P ( G ) = 1 , and The Diagonal Gaussian Random Series in a Hilbert Space: Almost Sure Convergence, Finite-Dimensional Projections, and the Unique Measure with Diagonal Gaussian Projections §random-element gives ⟨ Y , e k ⟩ = c k ξ k = : ζ k \langle Y,e_{k}\rangle=\sqrt{c_{k}}\xi_{k}=:\zeta_{k} ⟨ Y , e k ⟩ = c k ξ k =: ζ k on G G G . The ζ k \zeta_{k} ζ k (k ∈ [ d ] k\in[d] k ∈ [ d ] ) are independent (Independence of Events and of Random Variables ), since { ζ k ∈ B } = { ξ k ∈ B ′ } \{\zeta_{k}\in B\}=\{\xi_{k}\in B'\} { ζ k ∈ B } = { ξ k ∈ B ′ } with B ′ B' B ′ the preimage of B B B under the continuous map t ↦ c k t t\mapsto\sqrt{c_{k}}t t ↦ c k t . With ζ ( i ) = ( ζ j ) j ∈ I i \zeta^{(i)}=(\zeta_{j})_{j\in I_{i}} ζ ( i ) = ( ζ j ) j ∈ I i , claim 3 of Joint Distribution, Expectations, and Block Independence for Independent Random Variables , applied to the indicators 1 D i \mathbf{1}_{D_{i}} 1 D i (jointly Borel by claim 1 of Arithmetic, Absolute Values, and Pointwise Limits of Measurable Real-Valued Functions ), shows that 1 D 1 ( ζ ( 1 ) ) \mathbf{1}_{D_{1}}(\zeta^{(1)}) 1 D 1 ( ζ ( 1 ) ) and 1 D 2 ( ζ ( 2 ) ) \mathbf{1}_{D_{2}}(\zeta^{(2)}) 1 D 2 ( ζ ( 2 ) ) are independent, whence P ( ζ ( 1 ) ∈ D 1 , ζ ( 2 ) ∈ D 2 ) = P ( ζ ( 1 ) ∈ D 1 ) P ( ζ ( 2 ) ∈ D 2 ) P(\zeta^{(1)}\in D_{1},\zeta^{(2)}\in D_{2})=P(\zeta^{(1)}\in D_{1})P(\zeta^{(2)}\in D_{2}) P ( ζ ( 1 ) ∈ D 1 , ζ ( 2 ) ∈ D 2 ) = P ( ζ ( 1 ) ∈ D 1 ) P ( ζ ( 2 ) ∈ D 2 ) . Since π i ( Y ) = ζ ( i ) \pi_{i}(Y)=\zeta^{(i)} π i ( Y ) = ζ ( i ) on G G G and P ( Ω ∖ G ) = 0 P(\Omega\setminus G)=0 P ( Ω ∖ G ) = 0 , γ c ( A 1 ∩ A 2 ) = P ( π 1 ( Y ) ∈ D 1 , π 2 ( Y ) ∈ D 2 ) \gamma_{c}(A_{1}\cap A_{2})=P(\pi_{1}(Y)\in D_{1},\pi_{2}(Y)\in D_{2}) γ c ( A 1 ∩ A 2 ) = P ( π 1 ( Y ) ∈ D 1 , π 2 ( Y ) ∈ D 2 ) equals the left side and γ c ( A i ) = P ( ζ ( i ) ∈ D i ) \gamma_{c}(A_{i})=P(\zeta^{(i)}\in D_{i}) γ c ( A i ) = P ( ζ ( i ) ∈ D i ) . Consequently, if U U U is G 1 \mathcal{G}_{1} G 1 -measurable and W W W is G 2 \mathcal{G}_{2} G 2 -measurable, both integrable, then U , W U,W U , W are independent random variables on ( X , B ( X ) , γ c ) (X,\mathcal{B}(X),\gamma_{c}) ( X , B ( X ) , γ c ) (their events { U ∈ B } \{U\in B\} { U ∈ B } , { W ∈ B ′ ′ } \{W\in B''\} { W ∈ B ′′ } lie in G 1 \mathcal{G}_{1} G 1 , G 2 \mathcal{G}_{2} G 2 ), and by Expectation of a Product of Independent Random Variables
E [ U W ] = E [ U ] E [ W ] . (4.1) \mathbb{E}[UW]=\mathbb{E}[U]\,\mathbb{E}[W].\tag{4.1} E [ U W ] = E [ U ] E [ W ] . ( 4.1 )
Step 5 (Claim 2). We check (i)-(iii) of Conditional Expectation of a Square-Integrable Random Variable ; V M V_{M} V M and V N V_{N} V N are square-integrable by Step 3, and F N ⊆ B ( X ) \mathcal{F}_{N}\subseteq\mathcal{B}(X) F N ⊆ B ( X ) since the coordinate maps are Borel by Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §continuity . (i): by Step 3, V N V_{N} V N is a linear combination of products of maps x ↦ x j x\mapsto x_{j} x ↦ x j with j ∈ J N j\in J_{N} j ∈ J N , each F N \mathcal{F}_{N} F N -measurable, so V N V_{N} V N is F N \mathcal{F}_{N} F N -measurable by claims 1-3 of Arithmetic, Absolute Values, and Pointwise Limits of Measurable Real-Valued Functions . (iii): by (0.1), Hermite Polynomials: Low Orders, Derivatives, Recursion, Scaling, the Addition Formula, Gaussian Orthogonality and the Mehler Identity §addition with variances C N C_{N} C N and ϑ \vartheta ϑ (so C N + ϑ = C M C_{N}+\vartheta=C_{M} C N + ϑ = C M ), and H 0 ϑ = 1 H^{\vartheta}_{0}=1 H 0 ϑ = 1 ,
f M ( Φ M [ x ] ( z ) ) = f N ( Φ N [ x ] ( z ) ) + R ( x , z ) , R ( x , z ) = ∑ r ∈ { 2 , 4 } b r ∑ i = 0 r − 1 ( r i ) H i C N ( Φ N [ x ] ( z ) ) H r − i ϑ ( Ψ [ x ] ( z ) ) . f_{M}(\Phi_{M}[x](z))=f_{N}(\Phi_{N}[x](z))+R(x,z),\qquad R(x,z)=\sum_{r\in\{2,4\}}b_{r}\sum_{i=0}^{r-1}\binom{r}{i}H^{C_{N}}_{i}(\Phi_{N}[x](z))\,H^{\vartheta}_{r-i}(\Psi[x](z)). f M ( Φ M [ x ] ( z )) = f N ( Φ N [ x ] ( z )) + R ( x , z ) , R ( x , z ) = r ∈ { 2 , 4 } ∑ b r i = 0 ∑ r − 1 ( i r ) H i C N ( Φ N [ x ] ( z )) H r − i ϑ ( Ψ [ x ] ( z )) .
R R R is elementary, and V M − V N = ∫ Q R ( ⋅ , z ) d z V_{M}-V_{N}=\int_{Q}R(\cdot,z)\,dz V M − V N = ∫ Q R ( ⋅ , z ) d z by The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §potential and linearity of the integral; so for A ∈ F N A\in\mathcal{F}_{N} A ∈ F N , (0.2) gives E [ 1 A ( V M − V N ) ] = ∫ Q E [ 1 A R ( ⋅ , z ) ] d z \mathbb{E}[\mathbf{1}_{A}(V_{M}-V_{N})]=\int_{Q}\mathbb{E}[\mathbf{1}_{A}R(\cdot,z)]\,dz E [ 1 A ( V M − V N )] = ∫ Q E [ 1 A R ( ⋅ , z )] d z . Fix z z z and 0 ≤ i < r 0\le i<r 0 ≤ i < r , and put U = 1 A H i C N ( Φ N [ ⋅ ] ( z ) ) U=\mathbf{1}_{A}H^{C_{N}}_{i}(\Phi_{N}[\cdot](z)) U = 1 A H i C N ( Φ N [ ⋅ ] ( z )) and W = H r − i ϑ ( Ψ [ ⋅ ] ( z ) ) W=H^{\vartheta}_{r-i}(\Psi[\cdot](z)) W = H r − i ϑ ( Ψ [ ⋅ ] ( z )) , integrable by Step 0. If J N , M = ∅ J_{N,M}=\emptyset J N , M = ∅ then Ψ = 0 \Psi=0 Ψ = 0 , ϑ = 0 \vartheta=0 ϑ = 0 and W = 0 r − i = 0 W=0^{r-i}=0 W = 0 r − i = 0 by Hermite Polynomials: Low Orders, Derivatives, Recursion, Scaling, the Addition Formula, Gaussian Orthogonality and the Mehler Identity §low-orders . Otherwise U U U is F N \mathcal{F}_{N} F N -measurable and W W W is measurable for the σ \sigma σ -algebra generated by the coordinates with indices in J N , M J_{N,M} J N , M (claims 1-3 of Arithmetic, Absolute Values, and Pointwise Limits of Measurable Real-Valued Functions ), so Step 4 with d = d M d=d_{M} d = d M , I 1 = J N I_{1}=J_{N} I 1 = J N , I 2 = J N , M I_{2}=J_{N,M} I 2 = J N , M gives E [ U W ] = E [ U ] E [ W ] \mathbb{E}[UW]=\mathbb{E}[U]\mathbb{E}[W] E [ U W ] = E [ U ] E [ W ] , and by (1.1) and Wick Powers of Paley-Wiener Functionals: Expansion in Cylindrical Hermite Polynomials, the Covariance Formula, Continuity in the Vector, and Membership in the Chaos §covariance (with : ℓ g z 0 : = 1 {:}\ell_{g_{z}}^{0}{:}=1 : ℓ g z 0 : = 1 and r − i ≠ 0 r-i\neq0 r − i = 0 ), E [ W ] = ∫ X : ℓ g z r − i : : ℓ g z 0 : d γ c = 0 \mathbb{E}[W]=\int_{X}{:}\ell_{g_{z}}^{r-i}{:}\,{:}\ell_{g_{z}}^{0}{:}\,d\gamma_{c}=0 E [ W ] = ∫ X : ℓ g z r − i : : ℓ g z 0 : d γ c = 0 . Thus E [ 1 A R ( ⋅ , z ) ] = 0 \mathbb{E}[\mathbf{1}_{A}R(\cdot,z)]=0 E [ 1 A R ( ⋅ , z )] = 0 for every z z z , and E [ V M 1 A ] = E [ V N 1 A ] \mathbb{E}[V_{M}\mathbf{1}_{A}]=\mathbb{E}[V_{N}\mathbf{1}_{A}] E [ V M 1 A ] = E [ V N 1 A ] . This proves claim 2.
Step 6 (Second moments). By (0.3) applied to f L ( Φ L [ x ] ( z ) ) f L ′ ( Φ L ′ [ x ] ( w ) ) f_{L}(\Phi_{L}[x](z))f_{L'}(\Phi_{L'}[x](w)) f L ( Φ L [ x ] ( z )) f L ′ ( Φ L ′ [ x ] ( w )) , then (1.1), Wick Powers of Paley-Wiener Functionals: Expansion in Cylindrical Hermite Polynomials, the Covariance Formula, Continuity in the Vector, and Membership in the Chaos §covariance (mixed orders contribute 0 0 0 ) and Step 1,
E [ V L V L ′ ] = ∫ Q ∫ Q ( 24 b 4 2 K 4 + 2 b 2 2 K 2 ) d w d z , E [ D k L D k L ′ ] = ∫ Q ∫ Q ( 6 ϰ 2 K 3 + m 2 K ) ψ k ( z ) ψ k ( w ) d w d z , \mathbb{E}[V_{L}V_{L'}]=\int_{Q}\int_{Q}\bigl(24b_{4}^{2}\mathcal{K}^{4}+2b_{2}^{2}\mathcal{K}^{2}\bigr)\,dw\,dz,\qquad \mathbb{E}[D^{L}_{k}D^{L'}_{k}]=\int_{Q}\int_{Q}\bigl(6\varkappa^{2}\mathcal{K}^{3}+\mathfrak{m}^{2}\mathcal{K}\bigr)\psi_{k}(z)\psi_{k}(w)\,dw\,dz, E [ V L V L ′ ] = ∫ Q ∫ Q ( 24 b 4 2 K 4 + 2 b 2 2 K 2 ) d w d z , E [ D k L D k L ′ ] = ∫ Q ∫ Q ( 6 ϰ 2 K 3 + m 2 K ) ψ k ( z ) ψ k ( w ) d w d z ,
with K = K L ∧ L ′ ( z , w ) \mathcal{K}=\mathcal{K}_{L\wedge L'}(z,w) K = K L ∧ L ′ ( z , w ) ; below, ∬ \iint ∬ abbreviates this iterated integral ∫ Q ∫ Q ⋯ d w d z \int_{Q}\int_{Q}\cdots\,dw\,dz ∫ Q ∫ Q ⋯ d w d z . Expanding E [ ( V M − V N ) 2 ] = E [ V M 2 ] − 2 E [ V M V N ] + E [ V N 2 ] \mathbb{E}[(V_{M}-V_{N})^{2}]=\mathbb{E}[V_{M}^{2}]-2\mathbb{E}[V_{M}V_{N}]+\mathbb{E}[V_{N}^{2}] E [( V M − V N ) 2 ] = E [ V M 2 ] − 2 E [ V M V N ] + E [ V N 2 ] , and likewise for D k M − D k N D^{M}_{k}-D^{N}_{k} D k M − D k N , with 24 b 4 2 = 3 2 ϰ 2 24b_{4}^{2}=\frac{3}{2}\varkappa^{2} 24 b 4 2 = 2 3 ϰ 2 , 2 b 2 2 = 1 2 m 2 2b_{2}^{2}=\frac{1}{2}\mathfrak{m}^{2} 2 b 2 2 = 2 1 m 2 :
E [ ( V M − V N ) 2 ] = ∬ ( 3 2 ϰ 2 ( K M 4 − K N 4 ) + 1 2 m 2 ( K M 2 − K N 2 ) ) , E [ ( D k M − D k N ) 2 ] = ∬ ( 6 ϰ 2 ( K M 3 − K N 3 ) + m 2 ( K M − K N ) ) ψ k ( z ) ψ k ( w ) . \mathbb{E}[(V_{M}-V_{N})^{2}]=\iint\Bigl(\tfrac{3}{2}\varkappa^{2}(\mathcal{K}_{M}^{4}-\mathcal{K}_{N}^{4})+\tfrac{1}{2}\mathfrak{m}^{2}(\mathcal{K}_{M}^{2}-\mathcal{K}_{N}^{2})\Bigr),\quad \mathbb{E}[(D^{M}_{k}-D^{N}_{k})^{2}]=\iint\bigl(6\varkappa^{2}(\mathcal{K}_{M}^{3}-\mathcal{K}_{N}^{3})+\mathfrak{m}^{2}(\mathcal{K}_{M}-\mathcal{K}_{N})\bigr)\psi_{k}(z)\psi_{k}(w). E [( V M − V N ) 2 ] = ∬ ( 2 3 ϰ 2 ( K M 4 − K N 4 ) + 2 1 m 2 ( K M 2 − K N 2 ) ) , E [( D k M − D k N ) 2 ] = ∬ ( 6 ϰ 2 ( K M 3 − K N 3 ) + m 2 ( K M − K N ) ) ψ k ( z ) ψ k ( w ) .
For k 1 , … , k r ∈ Z n k_{1},\dots,k_{r}\in\mathbb{Z}^{n} k 1 , … , k r ∈ Z n put T ( k 1 , … , k r ) = ∫ Q ∏ i = 1 r ψ k i d λ Q T(k_{1},\dots,k_{r})=\int_{Q}\prod_{i=1}^{r}\psi_{k_{i}}\,d\lambda_{Q} T ( k 1 , … , k r ) = ∫ Q ∏ i = 1 r ψ k i d λ Q . Expanding K L r \mathcal{K}_{L}^{r} K L r by distributivity over Γ L r \Gamma_{L}^{r} Γ L r (Step 1) and integrating term by term,
∬ K L r = ∑ ( k i ) ∈ Γ L r ∏ i μ k i − 1 T ( k 1 , … , k r ) 2 , ∬ K L r ψ k ( z ) ψ k ( w ) = ∑ ( k i ) ∈ Γ L r ∏ i μ k i − 1 T ( k 1 , … , k r , k ) 2 . \iint\mathcal{K}_{L}^{r}=\sum_{(k_{i})\in\Gamma_{L}^{r}}\prod_{i}\mu_{k_{i}}^{-1}\,T(k_{1},\dots,k_{r})^{2},\qquad \iint\mathcal{K}_{L}^{r}\psi_{k}(z)\psi_{k}(w)=\sum_{(k_{i})\in\Gamma_{L}^{r}}\prod_{i}\mu_{k_{i}}^{-1}\,T(k_{1},\dots,k_{r},k)^{2}. ∬ K L r = ( k i ) ∈ Γ L r ∑ i ∏ μ k i − 1 T ( k 1 , … , k r ) 2 , ∬ K L r ψ k ( z ) ψ k ( w ) = ( k i ) ∈ Γ L r ∑ i ∏ μ k i − 1 T ( k 1 , … , k r , k ) 2 .
By The Trigonometric System on the Torus is Orthonormal §classes , The Lebesgue Space of Square-Integrable Functions is a Real Hilbert Space §inner-product and The Trigonometric System on the Torus is Orthonormal §orthonormal , T ( k , k ′ ) = ⟨ E k , E k ′ ⟩ L 2 T(k,k')=\langle E_{k},E_{k'}\rangle_{L^{2}} T ( k , k ′ ) = ⟨ E k , E k ′ ⟩ L 2 is 1 1 1 if k = k ′ k=k' k = k ′ and 0 0 0 otherwise. Put
Σ 4 = ∑ ( k i ) ∈ Γ M 4 ∖ Γ N 4 ∏ i = 1 4 μ k i − 1 T ( k 1 , k 2 , k 3 , k 4 ) 2 , Σ 2 = ∑ k ∈ Γ M ∖ Γ N μ k − 2 \Sigma_{4}=\sum_{(k_{i})\in\Gamma_{M}^{4}\setminus\Gamma_{N}^{4}}\prod_{i=1}^{4}\mu_{k_{i}}^{-1}\,T(k_{1},k_{2},k_{3},k_{4})^{2},\qquad \Sigma_{2}=\sum_{k\in\Gamma_{M}\setminus\Gamma_{N}}\mu_{k}^{-2} Σ 4 = ( k i ) ∈ Γ M 4 ∖ Γ N 4 ∑ i = 1 ∏ 4 μ k i − 1 T ( k 1 , k 2 , k 3 , k 4 ) 2 , Σ 2 = k ∈ Γ M ∖ Γ N ∑ μ k − 2
(empty sums being 0 0 0 ). As Γ N r ⊆ Γ M r \Gamma_{N}^{r}\subseteq\Gamma_{M}^{r} Γ N r ⊆ Γ M r and only diagonal pairs have T ( k , k ′ ) ≠ 0 T(k,k')\ne0 T ( k , k ′ ) = 0 ,
E [ ( V M − V N ) 2 ] = 3 2 ϰ 2 Σ 4 + 1 2 m 2 Σ 2 . (6.1) \mathbb{E}[(V_{M}-V_{N})^{2}]=\tfrac{3}{2}\varkappa^{2}\Sigma_{4}+\tfrac{1}{2}\mathfrak{m}^{2}\Sigma_{2}.\tag{6.1} E [( V M − V N ) 2 ] = 2 3 ϰ 2 Σ 4 + 2 1 m 2 Σ 2 . ( 6.1 )
For the derivatives, Step 2 gives for j ∈ [ d M ] j\in[d_{M}] j ∈ [ d M ] with k = κ ( j ) k=\kappa(j) k = κ ( j ) : ∂ j V M − ∂ j V N = a j − 1 / 2 ( D k M − D k N ) \partial_{j}V_{M}-\partial_{j}V_{N}=a_{j}^{-1/2}(D^{M}_{k}-D^{N}_{k}) ∂ j V M − ∂ j V N = a j − 1/2 ( D k M − D k N ) if j ∈ J N j\in J_{N} j ∈ J N , = a j − 1 / 2 D k M =a_{j}^{-1/2}D^{M}_{k} = a j − 1/2 D k M if j ∈ J N , M j\in J_{N,M} j ∈ J N , M , and = 0 =0 = 0 otherwise. With c j ( a j − 1 / 2 ) 2 = μ k − 1 c_{j}(a_{j}^{-1/2})^{2}=\mu_{k}^{-1} c j ( a j − 1/2 ) 2 = μ k − 1 and the bijections of Step 0,
∑ j = 1 d M c j E [ ( ∂ j V M − ∂ j V N ) 2 ] = ∑ k ∈ Γ N μ k − 1 E [ ( D k M − D k N ) 2 ] + ∑ k ∈ Γ M ∖ Γ N μ k − 1 E [ ( D k M ) 2 ] . \sum_{j=1}^{d_{M}}c_{j}\,\mathbb{E}[(\partial_{j}V_{M}-\partial_{j}V_{N})^{2}]=\sum_{k\in\Gamma_{N}}\mu_{k}^{-1}\mathbb{E}[(D^{M}_{k}-D^{N}_{k})^{2}]+\sum_{k\in\Gamma_{M}\setminus\Gamma_{N}}\mu_{k}^{-1}\mathbb{E}[(D^{M}_{k})^{2}]. j = 1 ∑ d M c j E [( ∂ j V M − ∂ j V N ) 2 ] = k ∈ Γ N ∑ μ k − 1 E [( D k M − D k N ) 2 ] + k ∈ Γ M ∖ Γ N ∑ μ k − 1 E [( D k M ) 2 ] .
For k ∈ Γ N k\in\Gamma_{N} k ∈ Γ N , ∬ ( K M − K N ) ψ k ( z ) ψ k ( w ) = ∑ k ′ ∈ Γ M ∖ Γ N μ k ′ − 1 T ( k ′ , k ) 2 = 0 \iint(\mathcal{K}_{M}-\mathcal{K}_{N})\psi_{k}(z)\psi_{k}(w)=\sum_{k'\in\Gamma_{M}\setminus\Gamma_{N}}\mu_{k'}^{-1}T(k',k)^{2}=0 ∬ ( K M − K N ) ψ k ( z ) ψ k ( w ) = ∑ k ′ ∈ Γ M ∖ Γ N μ k ′ − 1 T ( k ′ , k ) 2 = 0 , and the cubic part is 6 ϰ 2 6\varkappa^{2} 6 ϰ 2 times the sum over ( k 1 , k 2 , k 3 ) ∈ Γ M 3 ∖ Γ N 3 (k_{1},k_{2},k_{3})\in\Gamma_{M}^{3}\setminus\Gamma_{N}^{3} ( k 1 , k 2 , k 3 ) ∈ Γ M 3 ∖ Γ N 3 ; for k ∈ Γ M ∖ Γ N k\in\Gamma_{M}\setminus\Gamma_{N} k ∈ Γ M ∖ Γ N , E [ ( D k M ) 2 ] \mathbb{E}[(D^{M}_{k})^{2}] E [( D k M ) 2 ] is 6 ϰ 2 6\varkappa^{2} 6 ϰ 2 times the sum over Γ M 3 \Gamma_{M}^{3} Γ M 3 plus m 2 μ k − 1 \mathfrak{m}^{2}\mu_{k}^{-1} m 2 μ k − 1 . A tuple ( k 1 , k 2 , k 3 , k ) ∈ Γ M 4 (k_{1},k_{2},k_{3},k)\in\Gamma_{M}^{4} ( k 1 , k 2 , k 3 , k ) ∈ Γ M 4 lies outside Γ N 4 \Gamma_{N}^{4} Γ N 4 exactly when k ∈ Γ N k\in\Gamma_{N} k ∈ Γ N and ( k 1 , k 2 , k 3 ) ∉ Γ N 3 (k_{1},k_{2},k_{3})\notin\Gamma_{N}^{3} ( k 1 , k 2 , k 3 ) ∈ / Γ N 3 , or k ∉ Γ N k\notin\Gamma_{N} k ∈ / Γ N ; hence
∑ j = 1 d M c j E [ ( ∂ j V M − ∂ j V N ) 2 ] = 6 ϰ 2 Σ 4 + m 2 Σ 2 . (6.2) \sum_{j=1}^{d_{M}}c_{j}\,\mathbb{E}[(\partial_{j}V_{M}-\partial_{j}V_{N})^{2}]=6\varkappa^{2}\Sigma_{4}+\mathfrak{m}^{2}\Sigma_{2}.\tag{6.2} j = 1 ∑ d M c j E [( ∂ j V M − ∂ j V N ) 2 ] = 6 ϰ 2 Σ 4 + m 2 Σ 2 . ( 6.2 )
Step 7 (The quartic integrals). Let k = ( k 1 , … , k 4 ) ∈ ( Z n ) 4 k=(k_{1},\dots,k_{4})\in(\mathbb{Z}^{n})^{4} k = ( k 1 , … , k 4 ) ∈ ( Z n ) 4 , with k i , l k_{i,l} k i , l the l l l -th component of k i k_{i} k i . We show: (a) ∣ T ( k ) ∣ ≤ 4 n |T(k)|\le4^{n} ∣ T ( k ) ∣ ≤ 4 n ; (b) if T ( k ) ≠ 0 T(k)\ne0 T ( k ) = 0 , then for each l ∈ [ n ] l\in[n] l ∈ [ n ] there are ε 1 , l , … , ε 4 , l ∈ { 1 , − 1 } \varepsilon_{1,l},\dots,\varepsilon_{4,l}\in\{1,-1\} ε 1 , l , … , ε 4 , l ∈ { 1 , − 1 } with ∑ i ε i , l k i , l = 0 \sum_{i}\varepsilon_{i,l}k_{i,l}=0 ∑ i ε i , l k i , l = 0 . Let J 0 = { t : 0 ≤ t < 1 } J^{0}=\{t:0\le t<1\} J 0 = { t : 0 ≤ t < 1 } with the measure λ J 0 \lambda_{J^{0}} λ J 0 (the set J J J of The Integral over the Unit Cell of a Product of One-Variable Functions ), let ϕ m \phi_{m} ϕ m be the maps of The Trigonometric System on the Torus §one-dimensional , and g l ( t ) = ∏ i = 1 4 ϕ k i , l ( t ) g_{l}(t)=\prod_{i=1}^{4}\phi_{k_{i,l}}(t) g l ( t ) = ∏ i = 1 4 ϕ k i , l ( t ) . By The Trigonometric System on the Torus §system , ∏ i ψ k i ( z ) = ∏ l g l ( z l ) \prod_{i}\psi_{k_{i}}(z)=\prod_{l}g_{l}(z_{l}) ∏ i ψ k i ( z ) = ∏ l g l ( z l ) ; each ϕ m \phi_{m} ϕ m is a constant multiple of C ∣ m ∣ C_{|m|} C ∣ m ∣ or S ∣ m ∣ S_{|m|} S ∣ m ∣ (with C b , S b C_{b},S_{b} C b , S b as in Cell Integrals of the Trigonometric Monomials ; see (b) below), which is continuous on R \mathbb{R} R by Cell Integrals of the Trigonometric Monomials §calculus , so g l g_{l} g l , a product of such maps, is continuous by Continuity of Sums and Products of Real-Valued Functions on a Metric Space §on-set , hence measurable on J 0 J^{0} J 0 , and ∣ g l ∣ ≤ 4 |g_{l}|\le4 ∣ g l ∣ ≤ 4 by The Trigonometric System on the Torus is Orthonormal §derivative . So The Integral over the Unit Cell of a Product of One-Variable Functions §integral gives T ( k ) = ∏ l τ l T(k)=\prod_{l}\tau_{l} T ( k ) = ∏ l τ l with τ l = ∫ J 0 g l d λ J 0 \tau_{l}=\int_{J^{0}}g_{l}\,d\lambda_{J^{0}} τ l = ∫ J 0 g l d λ J 0 and ∣ τ l ∣ ≤ 4 λ J 0 ( J 0 ) = 4 |\tau_{l}|\le4\lambda_{J^{0}}(J^{0})=4 ∣ τ l ∣ ≤ 4 λ J 0 ( J 0 ) = 4 , proving (a). For (b), with C b , S b C_{b},S_{b} C b , S b as in Cell Integrals of the Trigonometric Monomials , each ϕ m \phi_{m} ϕ m is a constant multiple of C ∣ m ∣ C_{|m|} C ∣ m ∣ or S ∣ m ∣ S_{|m|} S ∣ m ∣ (ϕ 0 = 1 = C 0 \phi_{0}=1=C_{0} ϕ 0 = 1 = C 0 ). A product of factors C b i C_{b_{i}} C b i or S b i S_{b_{i}} S b i (i ≤ r i\le r i ≤ r , b i ∈ Z b_{i}\in\mathbb{Z} b i ∈ Z ) is a linear combination of maps C b C_{b} C b , S b S_{b} S b with b = ∑ i ε i b i b=\sum_{i}\varepsilon_{i}b_{i} b = ∑ i ε i b i for signs ε i \varepsilon_{i} ε i : induct on r r r , using (with u = 2 π b t u=2\pi bt u = 2 πb t , v = 2 π b ′ t v=2\pi b't v = 2 π b ′ t ) C b C b ′ = 1 2 ( C b − b ′ + C b + b ′ ) C_{b}C_{b'}=\frac12(C_{b-b'}+C_{b+b'}) C b C b ′ = 2 1 ( C b − b ′ + C b + b ′ ) , S b S b ′ = 1 2 ( C b − b ′ − C b + b ′ ) S_{b}S_{b'}=\frac12(C_{b-b'}-C_{b+b'}) S b S b ′ = 2 1 ( C b − b ′ − C b + b ′ ) , S b C b ′ = 1 2 ( S b + b ′ + S b − b ′ ) S_{b}C_{b'}=\frac12(S_{b+b'}+S_{b-b'}) S b C b ′ = 2 1 ( S b + b ′ + S b − b ′ ) from Product-to-Sum Formulas for Sine and Cosine §cosine-cosine , Product-to-Sum Formulas for Sine and Cosine §sine-sine , Product-to-Sum Formulas for Sine and Cosine §sine-cosine , and commutativity. By Cell Integrals of the Trigonometric Monomials §single , ∫ J 0 S b = 0 \int_{J^{0}}S_{b}=0 ∫ J 0 S b = 0 and ∫ J 0 C b = 0 \int_{J^{0}}C_{b}=0 ∫ J 0 C b = 0 unless b = 0 b=0 b = 0 . So T ( k ) ≠ 0 T(k)\neq0 T ( k ) = 0 forces each τ l ≠ 0 \tau_{l}\ne0 τ l = 0 , hence ∑ i ε i ′ ∣ k i , l ∣ = 0 \sum_{i}\varepsilon'_{i}|k_{i,l}|=0 ∑ i ε i ′ ∣ k i , l ∣ = 0 for some signs, and ε i , l = ε i ′ \varepsilon_{i,l}=\varepsilon'_{i} ε i , l = ε i ′ times the sign of k i , l k_{i,l} k i , l (1 1 1 if k i , l = 0 k_{i,l}=0 k i , l = 0 ) works.
Step 8 (Lattice bounds and claim 3). Put η = ( 4 π 2 ) − 1 / 8 \eta=(4\pi^{2})^{-1/8} η = ( 4 π 2 ) − 1/8 . If k ∈ Z n ∖ Γ N k\in\mathbb{Z}^{n}\setminus\Gamma_{N} k ∈ Z n ∖ Γ N , some component has ∣ k l ∣ ≥ N + 1 |k_{l}|\ge N+1 ∣ k l ∣ ≥ N + 1 , so μ k ≥ 4 π 2 k l 2 ≥ 4 π 2 N 2 \mu_{k}\ge4\pi^{2}k_{l}^{2}\ge4\pi^{2}N^{2} μ k ≥ 4 π 2 k l 2 ≥ 4 π 2 N 2 , and claims 1 and 2 of Real Powers Through the Exponential, and Elementary Asymptotic Tools: Monotonicity, Null Sequences of Negative Powers, Exponential Domination, Integer Rounding, and Square-Root and Exponential Inequalities give
μ k − 1 / 8 ≤ η N − 1 / 4 ( k ∉ Γ N ) . (8.1) \mu_{k}^{-1/8}\le\eta N^{-1/4}\qquad(k\notin\Gamma_{N}).\tag{8.1} μ k − 1/8 ≤ η N − 1/4 ( k ∈ / Γ N ) . ( 8.1 )
The sum Σ 2 \Sigma_{2} Σ 2 . Since μ k − 2 = μ k − 15 / 8 μ k − 1 / 8 \mu_{k}^{-2}=\mu_{k}^{-15/8}\mu_{k}^{-1/8} μ k − 2 = μ k − 15/8 μ k − 1/8 , (8.1) gives Σ 2 ≤ η N − 1 / 4 ∑ k ∈ Γ M μ k − 15 / 8 ≤ η N − 1 / 4 S 15 / 8 \Sigma_{2}\le\eta N^{-1/4}\sum_{k\in\Gamma_{M}}\mu_{k}^{-15/8}\le\eta N^{-1/4}S_{15/8} Σ 2 ≤ η N − 1/4 ∑ k ∈ Γ M μ k − 15/8 ≤ η N − 1/4 S 15/8 , where S 15 / 8 = ∑ k ∈ Z n μ k − 15 / 8 S_{15/8}=\sum_{k\in\mathbb{Z}^{n}}\mu_{k}^{-15/8} S 15/8 = ∑ k ∈ Z n μ k − 15/8 exists by Lattice Sums of Powers of the Fourier Weights in Dimension at Most Two: Power Sums, the Growth of the Wick Constants, and the Quartic Convolution Sums §powers (n ≤ 2 < 15 / 4 n\le2<15/4 n ≤ 2 < 15/4 ) and bounds the finite sums by Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §nonnegative .
The sum Σ 4 \Sigma_{4} Σ 4 . Let E \mathcal{E} E be the set of sign arrays ε = ( ε i , l ) ∈ { 1 , − 1 } 4 × n \varepsilon=(\varepsilon_{i,l})\in\{1,-1\}^{4\times n} ε = ( ε i , l ) ∈ { 1 , − 1 } 4 × n (16 n 16^{n} 1 6 n elements), and σ ε \sigma_{\varepsilon} σ ε the involution of ( Z n ) 4 (\mathbb{Z}^{n})^{4} ( Z n ) 4 multiplying the component k i , l k_{i,l} k i , l by ε i , l \varepsilon_{i,l} ε i , l . It preserves each μ k i \mu_{k_{i}} μ k i (a function of the squared components) and each Γ L 4 \Gamma_{L}^{4} Γ L 4 (defined by − L ≤ k i , l ≤ L -L\le k_{i,l}\le L − L ≤ k i , l ≤ L ), hence Δ = Γ M 4 ∖ Γ N 4 \Delta=\Gamma_{M}^{4}\setminus\Gamma_{N}^{4} Δ = Γ M 4 ∖ Γ N 4 . Let Z 0 = { k : ∑ i k i = 0 } Z_{0}=\{k:\sum_{i}k_{i}=0\} Z 0 = { k : ∑ i k i = 0 } . By Step 7(b), T ( k ) ≠ 0 T(k)\ne0 T ( k ) = 0 implies σ ε k ∈ Z 0 \sigma_{\varepsilon}k\in Z_{0} σ ε k ∈ Z 0 for some ε \varepsilon ε , and T ( k ) 2 ≤ 16 n T(k)^{2}\le16^{n} T ( k ) 2 ≤ 1 6 n by Step 7(a). Substituting k = σ ε k ′ k=\sigma_{\varepsilon}k' k = σ ε k ′ ,
Σ 4 ≤ 16 n ∑ ε ∈ E ∑ k ∈ Δ , σ ε k ∈ Z 0 ∏ i μ k i − 1 = 256 n ∑ k ′ ∈ Δ ∩ Z 0 ∏ i μ k i ′ − 1 . \Sigma_{4}\le16^{n}\sum_{\varepsilon\in\mathcal{E}}\ \sum_{k\in\Delta,\ \sigma_{\varepsilon}k\in Z_{0}}\prod_{i}\mu_{k_{i}}^{-1}=256^{n}\sum_{k'\in\Delta\cap Z_{0}}\prod_{i}\mu_{k'_{i}}^{-1}. Σ 4 ≤ 1 6 n ε ∈ E ∑ k ∈ Δ , σ ε k ∈ Z 0 ∑ i ∏ μ k i − 1 = 25 6 n k ′ ∈ Δ ∩ Z 0 ∑ i ∏ μ k i ′ − 1 .
Each k ′ ∈ Δ ∩ Z 0 k'\in\Delta\cap Z_{0} k ′ ∈ Δ ∩ Z 0 lies in Γ M 4 ∩ Z 0 \Gamma_{M}^{4}\cap Z_{0} Γ M 4 ∩ Z 0 with k i ′ ∉ Γ N k'_{i}\notin\Gamma_{N} k i ′ ∈ / Γ N for some i ∈ { 1 , 2 , 3 , 4 } i\in\{1,2,3,4\} i ∈ { 1 , 2 , 3 , 4 } , and there ∏ μ k i ′ ′ − 1 = μ k i ′ − 1 / 8 F i ( k 1 ′ , k 2 ′ , k 3 ′ ) ≤ η N − 1 / 4 F i ( k 1 ′ , k 2 ′ , k 3 ′ ) \prod\mu_{k'_{i'}}^{-1}=\mu_{k'_{i}}^{-1/8}F_{i}(k'_{1},k'_{2},k'_{3})\le\eta N^{-1/4}F_{i}(k'_{1},k'_{2},k'_{3}) ∏ μ k i ′ ′ − 1 = μ k i ′ − 1/8 F i ( k 1 ′ , k 2 ′ , k 3 ′ ) ≤ η N − 1/4 F i ( k 1 ′ , k 2 ′ , k 3 ′ ) by (8.1), where F i F_{i} F i is the family of Lattice Sums of Powers of the Fourier Weights in Dimension at Most Two: Power Sums, the Growth of the Wick Constants, and the Quartic Convolution Sums §quartic with δ = 1 / 8 \delta=1/8 δ = 1/8 (as k 4 ′ = − ( k 1 ′ + k 2 ′ + k 3 ′ ) k'_{4}=-(k'_{1}+k'_{2}+k'_{3}) k 4 ′ = − ( k 1 ′ + k 2 ′ + k 3 ′ ) ). The map k ′ ↦ ( k 1 ′ , k 2 ′ , k 3 ′ ) k'\mapsto(k'_{1},k'_{2},k'_{3}) k ′ ↦ ( k 1 ′ , k 2 ′ , k 3 ′ ) is a bijection of Γ M 4 ∩ Z 0 \Gamma_{M}^{4}\cap Z_{0} Γ M 4 ∩ Z 0 onto a nonempty finite subset of Z 3 n \mathbb{Z}^{3n} Z 3 n (it contains 0 0 0 ), so by Lattice Sums along Cubes: Linearity, Nonnegative Families, Absolute Summability, Comparison and Finitely Supported Families §nonnegative , with Λ i = ∑ Z 3 n F i \Lambda_{i}=\sum_{\mathbb{Z}^{3n}}F_{i} Λ i = ∑ Z 3 n F i the lattice sum given by Lattice Sums of Powers of the Fourier Weights in Dimension at Most Two: Power Sums, the Growth of the Wick Constants, and the Quartic Convolution Sums §quartic ,
Σ 4 ≤ 256 n η N − 1 / 4 ( Λ 1 + Λ 2 + Λ 3 + Λ 4 ) . \Sigma_{4}\le256^{n}\eta N^{-1/4}(\Lambda_{1}+\Lambda_{2}+\Lambda_{3}+\Lambda_{4}). Σ 4 ≤ 25 6 n η N − 1/4 ( Λ 1 + Λ 2 + Λ 3 + Λ 4 ) .
Conclusion. Put C = η ( 6 ϰ 2 256 n ( Λ 1 + Λ 2 + Λ 3 + Λ 4 ) + m 2 S 15 / 8 ) ≥ 0 C=\eta\bigl(6\varkappa^{2}256^{n}(\Lambda_{1}+\Lambda_{2}+\Lambda_{3}+\Lambda_{4})+\mathfrak{m}^{2}S_{15/8}\bigr)\ge0 C = η ( 6 ϰ 2 25 6 n ( Λ 1 + Λ 2 + Λ 3 + Λ 4 ) + m 2 S 15/8 ) ≥ 0 , which depends only on n n n , ϰ \varkappa ϰ and m \mathfrak{m} m (S 15 / 8 S_{15/8} S 15/8 and Λ i \Lambda_{i} Λ i depend on n n n only). Since Σ 4 , Σ 2 ≥ 0 \Sigma_{4},\Sigma_{2}\ge0 Σ 4 , Σ 2 ≥ 0 , (6.1) and (6.2) give that both quantities of claim 3 are at most 6 ϰ 2 Σ 4 + m 2 Σ 2 ≤ C N − 1 / 4 6\varkappa^{2}\Sigma_{4}+\mathfrak{m}^{2}\Sigma_{2}\le C\,N^{-1/4} 6 ϰ 2 Σ 4 + m 2 Σ 2 ≤ C N − 1/4 , for all N ≤ M N\le M N ≤ M . This proves claim 3.