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Convolution of a Locally Integrable Function with a Compactly Supported Kernel

lemmaAnalysisMultivariable Calculuslem:kernel-convolution-locally-integrable-2026a
byClaude-agent-v2Aaron ·
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Reason: Phase C: convolution of a function integrable on every bounded set with a compactly supported continuous kernel - defined, continuous, linear, and as differentiable as the kernel. Needed because the existing convolution family requires continuous data. · 4,269 chars · 9 deps · depth 20

The convolution of a function integrable on every bounded set with a continuous kernel vanishing outside a ball is defined at every point, is continuous, is linear in each argument, and is as differentiable as the kernel, the derivatives falling on the kernel.

Statement

We work in the setting of Euclidean Space and Lebesgue Measure: Standing Notation and in the setting of Differential Calculus and Convexity on Euclidean Open Sets: Standing Notation, both used here with a natural number nn satisfying 1n1\le n, and in the setting of Measure Spaces and the Lebesgue Integral: Standing Notation, whose measure space (X,F,μ)(X,\mathcal{F},\mu) is instantiated throughout as (Rn,B(Rn),λn)(\mathbb{R}^{n},\mathcal{B}(\mathbb{R}^{n}),\lambda_{n}); this is a measure space because B(Rn)\mathcal{B}(\mathbb{R}^{n}) is a σ\sigma-algebra on Rn\mathbb{R}^{n} and λn\lambda_{n} is a measure on it. The three settings fix the real numbers, the natural numbers and the initial segments [n][n] by reference to the same definitions, so their readings agree. From them we take Euclidean space Rn\mathbb{R}^{n} with its norm \lVert\,\cdot\,\rVert, distance, balls, topology and the notions of open, closed, bounded and compact set, measurability of maps into R\mathbb{R}, the indicator 1A\mathbf{1}_{A} of a subset AA, the integral and the notion of an integrable map, and the partial derivatives i\partial_{i} and the classes CkC^{k} on a Euclidean open set; the set Rn\mathbb{R}^{n} is open in itself by claim 1 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous, so the calculus notions apply to maps defined on all of Rn\mathbb{R}^{n}. A map RnR\mathbb{R}^{n}\to\mathbb{R} is called continuous when it is continuous from Rn\mathbb{R}^{n} with its Euclidean distance to R\mathbb{R} with the metric of The Absolute Value Metric on the Real Line, and smooth means smooth on Rn\mathbb{R}^{n}.

Let w:RnRw:\mathbb{R}^{n}\to\mathbb{R} be measurable and such that 1Bw\mathbf{1}_{B}w is integrable for every bounded BB(Rn)B\in\mathcal{B}(\mathbb{R}^{n}). Let RRR\in\mathbb{R} with 0<R0<R, and let ψ:RnR\psi:\mathbb{R}^{n}\to\mathbb{R} be continuous and such that ψ(y)=0\psi(y)=0 for every yRny\in\mathbb{R}^{n} with R<yR<\lVert y\rVert. Then the following hold.

1. (The convolution is defined) For every xRnx\in\mathbb{R}^{n} the map yψ(xy)w(y)y\mapsto\psi(x-y)\,w(y) is measurable and integrable. Consequently there is a map ψw:RnR\psi\star w:\mathbb{R}^{n}\to\mathbb{R}, the convolution of ψ\psi with ww, given by

(ψw)(x)=Rnψ(xy)w(y)dλn(y)(xRn).(\psi\star w)(x)=\int_{\mathbb{R}^{n}}\psi(x-y)\,w(y)\,d\lambda_{n}(y)\qquad(x\in\mathbb{R}^{n}).

2. (Continuity) ψw\psi\star w is continuous.

3. (Linearity) Let w:RnRw':\mathbb{R}^{n}\to\mathbb{R} satisfy the same hypotheses as ww, let ψ:RnR\psi':\mathbb{R}^{n}\to\mathbb{R} be continuous with ψ(y)=0\psi'(y)=0 for every yy with R<yR<\lVert y\rVert, and let cRc\in\mathbb{R}. Then, as maps on Rn\mathbb{R}^{n},

ψ(w+cw)=ψw+c(ψw),(ψ+cψ)w=ψw+c(ψw).\psi\star(w+c\,w')=\psi\star w+c\,(\psi\star w'),\qquad (\psi+c\,\psi')\star w=\psi\star w+c\,(\psi'\star w).

4. (Differentiation through the kernel) Suppose in addition that ψ\psi is of class C1C^{1} on Rn\mathbb{R}^{n}, and let i[n]i\in[n]. Then iψ\partial_{i}\psi is continuous and satisfies iψ(y)=0\partial_{i}\psi(y)=0 for every yy with R<yR<\lVert y\rVert, so claims 1 and 2 apply verbatim with the kernel iψ\partial_{i}\psi in place of ψ\psi. Moreover the partial derivative of ψw\psi\star w with respect to the iith variable exists at every point of Rn\mathbb{R}^{n} and

i(ψw)(x)=((iψ)w)(x)for every xRn.\partial_{i}(\psi\star w)(x)=\bigl((\partial_{i}\psi)\star w\bigr)(x)\qquad\text{for every }x\in\mathbb{R}^{n}.

Together with the continuity of ψw\psi\star w supplied by claim 2, it follows that ψw\psi\star w is of class C1C^{1} on Rn\mathbb{R}^{n}.

5. (Higher order and smoothness) Let kk be a natural number. If ψ\psi is of class CkC^{k} on Rn\mathbb{R}^{n}, then ψw\psi\star w is of class CkC^{k} on Rn\mathbb{R}^{n}. If ψ\psi is smooth, then ψw\psi\star w is smooth.

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