In the setting of Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation , with the coordinates x k x_{k} x k , the maps Q n Q_{n} Q n and the spans X n X_{n} X n of Borel Probability Measures on a Real Hilbert Space with an Orthonormal Basis: Standing Notation §coordinates , let μ \mu μ belong to the set P 2 ( X ) \mathcal{P}_{2}(X) P 2 ( X ) of The Second Moment of a Borel Probability Measure on a Hilbert Space and the Probability Measures with Finite Second Moment §space and let n ∈ N n\in\mathbb{N} n ∈ N . Throughout, the dimension written d d d or q q q in the Euclidean items cited below is n n n , and the letter d d d is kept for the distance of X X X . For k ∈ N k\in\mathbb{N} k ∈ N , a k 1 / 2 a_{k}^{1/2} a k 1/2 is the positive square root of the noise weight a k a_{k} a k given by Existence and Uniqueness of the Nonnegative Square Root , and a k − 1 / 2 a_{k}^{-1/2} a k − 1/2 is its multiplicative inverse. The rescaled head map is r n : X → R n r_{n}:X\to\mathbb{R}^{n} r n : X → R n ,
r n ( x ) = ( a 1 − 1 / 2 x 1 , … , a n − 1 / 2 x n ) ( x ∈ X ) , r_{n}(x)=\bigl(a_{1}^{-1/2}x_{1},\dots,a_{n}^{-1/2}x_{n}\bigr)\qquad(x\in X), r n ( x ) = ( a 1 − 1/2 x 1 , … , a n − 1/2 x n ) ( x ∈ X ) ,
and μ ~ = ( r n ) # μ \tilde{\mu}=(r_{n})_{\#}\mu μ ~ = ( r n ) # μ is its push-forward of Borel Probability Measures on a Real Hilbert Space with an Orthonormal Basis: Standing Notation §pushforward , defined because r n r_{n} r n is Borel by claim 1. For a probability measure λ \lambda λ on R n \mathbb{R}^{n} R n , L 2 ( λ ; R n ) L^{2}(\lambda;\mathbb{R}^{n}) L 2 ( λ ; R n ) is the space of square-integrable vector fields against λ \lambda λ , with inner product ⟨ ⋅ , ⋅ ⟩ λ \langle\cdot,\cdot\rangle_{\lambda} ⟨ ⋅ , ⋅ ⟩ λ ; for a test function ψ ∈ C c ∞ ( R n ) \psi\in C_{c}^{\infty}(\mathbb{R}^{n}) ψ ∈ C c ∞ ( R n ) the gradient map ∇ ψ \nabla\psi ∇ ψ is Borel with ∫ R n ∥ ∇ ψ ∥ 2 d λ < ∞ \int_{\mathbb{R}^{n}}\lVert\nabla\psi\rVert^{2}\,d\lambda<\infty ∫ R n ∥ ∇ ψ ∥ 2 d λ < ∞ by Square-Integrable Vector Fields Against a Probability Measure on Euclidean Space, and Test Functions: Standing Notation §test ; and for λ \lambda λ in the set P 2 ( R n ) \mathcal{P}_{2}(\mathbb{R}^{n}) P 2 ( R n ) of The Second Moment of a Probability Measure on Euclidean Space and the Probability Measures with Finite Second Moment §space , T λ T_{\lambda} T λ is the tangent space at λ \lambda λ . L 2 ( μ ; X a ) L^{2}(\mu;X^{a}) L 2 ( μ ; X a ) is the space of Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation §fields , with inner product ⟨ ⋅ , ⋅ ⟩ μ \langle\cdot,\cdot\rangle_{\mu} ⟨ ⋅ , ⋅ ⟩ μ ; F C b 1 ( X ) \mathcal{F}C^{1}_{b}(X) F C b 1 ( X ) is the set of bounded C 1 C^{1} C 1 cylindrical functions , ∇ a φ \nabla_{a}\varphi ∇ a φ is the noise gradient of φ ∈ F C b 1 ( X ) \varphi\in\mathcal{F}C^{1}_{b}(X) φ ∈ F C b 1 ( X ) , and T μ a T^{a}_{\mu} T μ a is the noise tangent space at μ \mu μ . For a Borel map η : R n → R n \eta:\mathbb{R}^{n}\to\mathbb{R}^{n} η : R n → R n with coordinates η 1 , … , η n \eta_{1},\dots,\eta_{n} η 1 , … , η n , its lift is the map Λ n η : X → X \Lambda_{n}\eta:X\to X Λ n η : X → X ,
Λ n η ( x ) = ∑ k = 1 n a k 1 / 2 η k ( r n ( x ) ) e k ( x ∈ X ) . \Lambda_{n}\eta(x)=\sum_{k=1}^{n}a_{k}^{1/2}\,\eta_{k}\bigl(r_{n}(x)\bigr)\,e_{k}\qquad(x\in X). Λ n η ( x ) = k = 1 ∑ n a k 1/2 η k ( r n ( x ) ) e k ( x ∈ X ) .
1. (The rescaled head) ¶ r n r_{n} r n is continuous from ( X , d ) (X,d) ( X , d ) to ( R n , d E ) (\mathbb{R}^{n},d_{E}) ( R n , d E ) , hence Borel , and μ ~ ∈ P 2 ( R n ) \tilde{\mu}\in\mathcal{P}_{2}(\mathbb{R}^{n}) μ ~ ∈ P 2 ( R n ) .
2. (The lift) ¶ Let η : R n → R n \eta:\mathbb{R}^{n}\to\mathbb{R}^{n} η : R n → R n be Borel with ∫ R n ∥ η ∥ 2 d μ ~ < ∞ \int_{\mathbb{R}^{n}}\lVert\eta\rVert^{2}\,d\tilde{\mu}<\infty ∫ R n ∥ η ∥ 2 d μ ~ < ∞ . Then Λ n η \Lambda_{n}\eta Λ n η is Borel as a map from X X X to X X X , takes its values in X n X_{n} X n and in X a X^{a} X a , is measurable as a map into X a X^{a} X a , and satisfies ∣ Λ n η ( x ) ∣ a 2 = ∥ η ( r n ( x ) ) ∥ 2 |\Lambda_{n}\eta(x)|_{a}^{2}=\lVert\eta(r_{n}(x))\rVert^{2} ∣ Λ n η ( x ) ∣ a 2 = ∥ η ( r n ( x )) ∥ 2 for every x ∈ X x\in X x ∈ X ; in particular it is square-integrable with respect to μ \mu μ . Its class in L 2 ( μ ; X a ) L^{2}(\mu;X^{a}) L 2 ( μ ; X a ) depends only on the class of η \eta η in L 2 ( μ ~ ; R n ) L^{2}(\tilde{\mu};\mathbb{R}^{n}) L 2 ( μ ~ ; R n ) , and the induced map, again written Λ n : L 2 ( μ ~ ; R n ) → L 2 ( μ ; X a ) \Lambda_{n}:L^{2}(\tilde{\mu};\mathbb{R}^{n})\to L^{2}(\mu;X^{a}) Λ n : L 2 ( μ ~ ; R n ) → L 2 ( μ ; X a ) , is linear and satisfies
⟨ Λ n ξ , Λ n η ⟩ μ = ⟨ ξ , η ⟩ μ ~ for all ξ , η ∈ L 2 ( μ ~ ; R n ) . \langle\Lambda_{n}\xi,\Lambda_{n}\eta\rangle_{\mu}=\langle\xi,\eta\rangle_{\tilde{\mu}}\qquad\text{for all }\xi,\eta\in L^{2}(\tilde{\mu};\mathbb{R}^{n}). ⟨ Λ n ξ , Λ n η ⟩ μ = ⟨ ξ , η ⟩ μ ~ for all ξ , η ∈ L 2 ( μ ~ ; R n ) .
3. (Shifted heads and tails) ¶ Let η : R n → R n \eta:\mathbb{R}^{n}\to\mathbb{R}^{n} η : R n → R n be Borel. Then for every x ∈ X x\in X x ∈ X
r n ( x + Λ n η ( x ) ) = r n ( x ) + η ( r n ( x ) ) , Q n ( x + Λ n η ( x ) ) = Q n x . r_{n}\bigl(x+\Lambda_{n}\eta(x)\bigr)=r_{n}(x)+\eta\bigl(r_{n}(x)\bigr),\qquad Q_{n}\bigl(x+\Lambda_{n}\eta(x)\bigr)=Q_{n}x . r n ( x + Λ n η ( x ) ) = r n ( x ) + η ( r n ( x ) ) , Q n ( x + Λ n η ( x ) ) = Q n x .
4. (Gradients) ¶ Let ψ ∈ C c ∞ ( R n ) \psi\in C_{c}^{\infty}(\mathbb{R}^{n}) ψ ∈ C c ∞ ( R n ) . Then ψ ∘ r n ∈ F C b 1 ( X ) \psi\circ r_{n}\in\mathcal{F}C^{1}_{b}(X) ψ ∘ r n ∈ F C b 1 ( X ) and Λ n ( ∇ ψ ) ( x ) = ∇ a ( ψ ∘ r n ) ( x ) \Lambda_{n}(\nabla\psi)(x)=\nabla_{a}(\psi\circ r_{n})(x) Λ n ( ∇ ψ ) ( x ) = ∇ a ( ψ ∘ r n ) ( x ) for every x ∈ X x\in X x ∈ X .
5. (Tangent fields) ¶ Λ n \Lambda_{n} Λ n maps T μ ~ T_{\tilde{\mu}} T μ ~ into T μ a T^{a}_{\mu} T μ a : if η ∈ T μ ~ \eta\in T_{\tilde{\mu}} η ∈ T μ ~ , then Λ n η ∈ T μ a \Lambda_{n}\eta\in T^{a}_{\mu} Λ n η ∈ T μ a .