Let n n n be a natural number with 1 ≤ n 1\le n 1 ≤ n , let R \mathbb{R} R be the real numbers with the order ≤ \le ≤ of their ordered field structure, write s < t s<t s < t to mean that s ≤ t s\le t s ≤ t and s ≠ t s\ne t s = t , write t − 1 t^{-1} t − 1 for the multiplicative inverse of t ≠ 0 t\ne 0 t = 0 , let ∣ s ∣ |s| ∣ s ∣ be the absolute value of s s s , and let d R d_{\mathbb{R}} d R be the metric on R \mathbb{R} R of The Absolute Value Metric on the Real Numbers . Let ∥ ⋅ ∥ \lVert\,\cdot\,\rVert ∥ ⋅ ∥ be the Euclidean norm on Euclidean space R n \mathbb{R}^{n} R n and let d d d be the Euclidean distance , a metric on R n \mathbb{R}^{n} R n ; by The Open Subsets of a Metric Space Form a Topology the subsets open in ( R n , d ) (\mathbb{R}^{n},d) ( R n , d ) form a topology, to which the topological notions below refer. Write B ˉ ( x , r ) \bar B(x,r) B ˉ ( x , r ) for the closed ball in ( R n , d ) (\mathbb{R}^{n},d) ( R n , d ) and let λ n \lambda_{n} λ n be Lebesgue measure on the Borel σ \sigma σ -algebra of R n \mathbb{R}^{n} R n . Powers with a natural exponent are those of Natural Number Power of an Element of a Field , and t y t\,y t y denotes the scalar multiple of y ∈ R n y\in\mathbb{R}^{n} y ∈ R n in the real vector space R n \mathbb{R}^{n} R n .
Let Ω ⊆ R n \Omega\subseteq\mathbb{R}^{n} Ω ⊆ R n be open in ( R n , d ) (\mathbb{R}^{n},d) ( R n , d ) and let f : Ω → R f:\Omega\to\mathbb{R} f : Ω → R be continuous on Ω \Omega Ω as a map from ( R n , d ) (\mathbb{R}^{n},d) ( R n , d ) into ( R , d R ) (\mathbb{R},d_{\mathbb{R}}) ( R , d R ) . Let δ ∈ R \delta\in\mathbb{R} δ ∈ R with 0 < δ 0<\delta 0 < δ and let ρ \rho ρ be a mollifier kernel of radius δ \delta δ on R n \mathbb{R}^{n} R n . For ε ∈ R \varepsilon\in\mathbb{R} ε ∈ R with 0 < ε 0<\varepsilon 0 < ε let ρ ε : R n → R \rho_{\varepsilon}:\mathbb{R}^{n}\to\mathbb{R} ρ ε : R n → R be given by ρ ε ( y ) = ( ε − 1 ) n ρ ( ε − 1 y ) \rho_{\varepsilon}(y)=(\varepsilon^{-1})^{n}\rho(\varepsilon^{-1}y) ρ ε ( y ) = ( ε − 1 ) n ρ ( ε − 1 y ) , a mollifier kernel of radius ε δ \varepsilon\delta ε δ by Rescaling a Mollifier Kernel ; being smooth it is continuous on R n \mathbb{R}^{n} R n by claim 3 of Euclidean Space is Open in Itself, and C k C^k C k Maps are Continuous and it vanishes at every y y y with ε δ < ∥ y ∥ \varepsilon\delta<\lVert y\rVert ε δ < ∥ y ∥ , so the convolution f ∗ ρ ε f*\rho_{\varepsilon} f ∗ ρ ε is defined, with kernel radius ε δ \varepsilon\delta ε δ , on the set Ω ε δ = { x ∈ R n : B ˉ ( x , ε δ ) ⊆ Ω } \Omega^{\varepsilon\delta}=\{x\in\mathbb{R}^{n}:\bar B(x,\varepsilon\delta)\subseteq\Omega\} Ω ε δ = { x ∈ R n : B ˉ ( x , ε δ ) ⊆ Ω } .
Let K ⊆ Ω K\subseteq\Omega K ⊆ Ω be compact in R n \mathbb{R}^{n} R n .
Then the following hold.
1. (The convolution is eventually defined on K K K ) There is ε 1 ∈ R \varepsilon_{1}\in\mathbb{R} ε 1 ∈ R with 0 < ε 1 0<\varepsilon_{1} 0 < ε 1 such that K ⊆ Ω ε δ K\subseteq\Omega^{\varepsilon\delta} K ⊆ Ω ε δ for every ε ∈ R \varepsilon\in\mathbb{R} ε ∈ R with 0 < ε ≤ ε 1 0<\varepsilon\le\varepsilon_{1} 0 < ε ≤ ε 1 .
2. (Uniform convergence on K K K ) For every η ∈ R \eta\in\mathbb{R} η ∈ R with 0 < η 0<\eta 0 < η there is ε 0 ∈ R \varepsilon_{0}\in\mathbb{R} ε 0 ∈ R with 0 < ε 0 0<\varepsilon_{0} 0 < ε 0 such that, for every ε ∈ R \varepsilon\in\mathbb{R} ε ∈ R with 0 < ε < ε 0 0<\varepsilon<\varepsilon_{0} 0 < ε < ε 0 , one has K ⊆ Ω ε δ K\subseteq\Omega^{\varepsilon\delta} K ⊆ Ω ε δ and
∣ ( f ∗ ρ ε ) ( x ) − f ( x ) ∣ < η for every x ∈ K . \bigl|(f*\rho_{\varepsilon})(x)-f(x)\bigr|<\eta\qquad\text{for every }x\in K . ( f ∗ ρ ε ) ( x ) − f ( x ) < η for every x ∈ K .