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The Lebesgue Bound for Periodic Convolution and Convergence of Mollifications

Periodic convolution is bounded on every Lebesgue space of the torus by the mass of its kernel, the mollifications of a power-integrable function converge to it in that space, and the smooth periodic functions are dense there.

Statement

We work in the setting of The Flat Torus: Standing Notation, used here with a natural number nn satisfying 1≤n1\le n and a real number pp with 1≤p1\le p; the cell QQ, the measure space (Q,BQ,λQ)(Q,\mathcal{B}_{Q},\lambda_{Q}), the classes Lp(Tn)\mathcal{L}^{p}(\mathbb{T}^{n}) and Lp(Tn)L^{p}(\mathbb{T}^{n}) with the class map [ ⋅ ][\,\cdot\,], the periodic classes CperC_{\mathrm{per}} and Cper∞C^{\infty}_{\mathrm{per}}, the restriction v∣Qv|_{Q}, and λn\lambda_{n} and the Euclidean norm ∥ ⋅ ∥\lVert\,\cdot\,\rVert are the ones fixed there. Let ∥ ⋅ ∥r\lVert\,\cdot\,\rVert_{r} denote the LrL^{r} seminorm of (Q,BQ,λQ)(Q,\mathcal{B}_{Q},\lambda_{Q}) for a real number rr with 1≤r1\le r, and let ψ⋆u\psi\star u denote the periodic convolution. Continuity and smoothness of a map on Rn\mathbb{R}^{n} are read as in Periodic Convolution and Mollification on the Torus.

Throughout, RR is a real number with 0<R0<R, the map ψ:Rn→R\psi:\mathbb{R}^{n}\to\mathbb{R} is continuous with ψ(y)=0\psi(y)=0 for every y∈Rny\in\mathbb{R}^{n} satisfying R<∥y∥R<\lVert y\rVert, and KK denotes the integral of ∣ψ∣|\psi| over Rn\mathbb{R}^{n}, a nonnegative real number by that clause. Then the following hold.

1. (The Lebesgue bound) Let u∈Lp(Tn)u\in\mathcal{L}^{p}(\mathbb{T}^{n}). Then (ψ⋆u)∣Q∈Lp(Tn)(\psi\star u)|_{Q}\in\mathcal{L}^{p}(\mathbb{T}^{n}) and

∥(ψ⋆u)∣Q∥p≤K ∥u∥p.\bigl\lVert(\psi\star u)|_{Q}\bigr\rVert_{p}\le K\,\lVert u\rVert_{p}.

2. (Convergence of the mollifications) Let δ∈R\delta\in\mathbb{R} with 0<δ0<\delta, let ρ\rho be a mollifier kernel of radius δ\delta on Rn\mathbb{R}^{n}, let u∈Lp(Tn)u\in\mathcal{L}^{p}(\mathbb{T}^{n}), and for a real number ε\varepsilon with 0<ε0<\varepsilon let ρε⋆u\rho_{\varepsilon}\star u be the mollification of uu of parameter ε\varepsilon by ρ\rho. Then for every real number η\eta with 0<η0<\eta there is a real number ε0\varepsilon_{0} with 0<ε00<\varepsilon_{0} such that

∥(ρε⋆u)∣Q−u∥p≤ηfor every real ε with 0<ε<ε0.\bigl\lVert(\rho_{\varepsilon}\star u)|_{Q}-u\bigr\rVert_{p}\le\eta\qquad\text{for every real }\varepsilon\text{ with }0<\varepsilon<\varepsilon_{0}.

Consequently the sequence whose kkth term is the class of (ρ1/k⋆u)∣Q(\rho_{1/k}\star u)|_{Q}, for kk a natural number, converges to [u][u] in Lp(Tn)L^{p}(\mathbb{T}^{n}).

3. (Smooth periodic functions are dense) The set {[w∣Q]:w∈Cper∞}\{[w|_{Q}]:w\in C^{\infty}_{\mathrm{per}}\} is dense in Lp(Tn)L^{p}(\mathbb{T}^{n}).

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