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Proof of The Mean L1L^1 Distance Between the Mollified Empirical Measure and the Mollified Measure

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Inside the ball of radius R, the empirical-average variance lemma bounds the mean-square fluctuation at each point by S eps−d/Neps^{-d}/N times the mollified density, and an optimised arithmetic-geometric mean inequality converts this into the square-root term; outside the ball, both mollified densities carry only mass coming from points of norm larger than R-1, which the particle laws and Markov's inequality bound by M2(mu)/(R−1)2M_2(mu)/(R-1)^2 each.

Proof

Each result cited is universally quantified over the data in its own statement, and is applied to the data named here. The field axioms and the rules for adding inequalities, for multiplying them by nonnegative or positive real numbers, and for handling absolute values, from Elementary Order Arithmetic in an Ordered Field, Elementary Arithmetic in an Ordered Field and Properties of the Absolute Value in an Ordered Field, are used without further mention; so are the facts that a square of a real number is nonnegative (claim 2 of Nonnegativity of Squares in an Ordered Field), that ∣t∣2=t2|t|^{2}=t^{2}, and that for nonnegative reals s,ts,t one has s<ts<t exactly when s2<t2s^{2}<t^{2} (Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field), and that 0<cn0<c^{n} for real c>0c>0 and natural nn (claims 5 and 4 of Properties of Natural Number Powers in a Field). For the Euclidean norm we use dE(y,y′)=∥y−y′∥d_{E}(y,y')=\lVert y-y'\rVert (claim 2 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n) and the triangle inequality (claim 6 there). Integrals of nonnegative measurable functions obey claim 1 of Linearity and Monotonicity of the Lebesgue Integral and those of integrable functions obey claim 2 there. For a nonnegative integrable function its real integral equals its integral as a nonnegative measurable function, the positive part being the function and the negative part 00 (Integrable Function and the Lebesgue Integral); conversely a nonnegative measurable real function with finite integral is integrable (Measure Spaces and the Lebesgue Integral: Standing Notation §integral). These facts are used without further mention.

Step 0 (Notation). Write Q=μ⊗NQ=\mu^{\otimes N}, a=ηε∗μa=\eta_{\varepsilon}*\mu and, for x∈RdNx\in\mathbb{R}^{dN}, ax=ηε∗μxNa_{x}=\eta_{\varepsilon}*\mu^{N}_{x}, which is defined since μxN∈P(Rd)\mu^{N}_{x}\in\mathcal{P}(\mathbb{R}^{d}) by The Empirical Measure of a Configuration of N Particles §empirical. By Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §density, aa and every axa_{x} are Borel, nonnegative and integrable with respect to λd\lambda_{d} with integral 11. Put cε=(ε−1)dc_{\varepsilon}=(\varepsilon^{-1})^{d}, v=S cεN−1v=S\,c_{\varepsilon}N^{-1} and c=κdRdc=\kappa_{d}R^{d}; these are positive, since 0<ε−10<\varepsilon^{-1}, 0<S0<S, 0<N−10<N^{-1} (claim 3 of Properties of the Canonical Map from the Natural Numbers to an Ordered Field), 0<κd0<\kappa_{d} (The Lebesgue Measure of a Closed Ball in Rn\mathbb{R}^n §constant) and 0<R0<R. Let B=Bˉ(0,R)B=\bar{B}(0,R); it is Borel with λd(B)=c\lambda_{d}(B)=c by The Lebesgue Measure of a Closed Ball in Rn\mathbb{R}^n §borel and The Lebesgue Measure of a Closed Ball in Rn\mathbb{R}^n §value, and Bc=Rd∖BB^{c}=\mathbb{R}^{d}\setminus B is Borel; a point yy lies in BcB^{c} exactly when R<dE(0,y)=∥y∥R<d_{E}(0,y)=\lVert y\rVert. The measures QQ and μ\mu are probability measures and λd\lambda_{d} is σ\sigma-finite by Lebesgue Measure on Euclidean Space is Sigma-Finite §sigma-finite, so the Tonelli statement of Tonelli and Fubini Theorems applies to each of the pairs (Q,λd)(Q,\lambda_{d}) and (μ,λd)(\mu,\lambda_{d}), with the Borel σ\sigma-algebras. For every λ∈R\lambda\in\mathbb{R}, ∑k=1Nλ=λN\sum_{k=1}^{N}\lambda=\lambda N by claim 3 of Properties of Finite Sums and The Canonical Map from the Natural Numbers to a Field.

Step 1 (Measurability). Let x∈RdNx\in\mathbb{R}^{dN} and y∈Rdy\in\mathbb{R}^{d}. The function x′↦ηε(y−x′)x'\mapsto\eta_{\varepsilon}(y-x') is Borel by Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §density, so Basic Properties of Empirical Measures: Values, Integrals, Push-Forwards, Second Moment, and Lipschitz Dependence on the Configuration §integral (with q=dq=d) gives

ax(y)=1N∑k=1Nηε(y−pk(x)),(1)a_{x}(y)=\frac{1}{N}\sum_{k=1}^{N}\eta_{\varepsilon}\bigl(y-\mathfrak{p}_{k}(x)\bigr),\tag{1}

with the block maps pk\mathfrak{p}_{k} of Particle Blocks of the Configuration Space: Block Maps, Configurations, Product Maps and Diagonal Points §blocks. Let P1=pr1dN,dP_{1}=\mathrm{pr}^{dN,d}_{1}, P2=pr2dN,dP_{2}=\mathrm{pr}^{dN,d}_{2} and ι=ιdN,d\iota=\iota^{dN,d} be the coordinate projections of RdN+d\mathbb{R}^{dN+d} and the concatenation (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pairs). The maps pk∘P1\mathfrak{p}_{k}\circ P_{1} and P2P_{2} are Borel, by Particle Blocks: Linearity, Splitting of Inner Products, Product Maps and Diagonal Shifts §linear, Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §projections and composition (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §borel-maps); so by Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §kernel (with m=dN+dm=dN+d) and claim 2 of Arithmetic, Absolute Values, and Pointwise Limits of Measurable Real-Valued Functions, the function Δ^(w)=∑k=1NN−1ηε(P2(w)−pk(P1(w)))−a(P2(w))\hat{\Delta}(w)=\sum_{k=1}^{N}N^{-1}\eta_{\varepsilon}(P_{2}(w)-\mathfrak{p}_{k}(P_{1}(w)))-a(P_{2}(w)) is Borel on RdN+d\mathbb{R}^{dN+d}, and so are ∣Δ^∣|\hat{\Delta}|, Δ^2\hat{\Delta}^{2} (claims 4 and 3 there), w↦1Bc(P2(w))w\mapsto\mathbf{1}_{B^{c}}(P_{2}(w)), which is the indicator of the Borel set P2−1(Bc)P_{2}^{-1}(B^{c}) (claim 1 there), and the products of the latter with ∣Δ^∣|\hat\Delta|, with ∑kN−1ηε(P2−pk∘P1)\sum_{k}N^{-1}\eta_{\varepsilon}(P_{2}-\mathfrak{p}_{k}\circ P_{1}) and with a∘P2a\circ P_{2}. By Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §product, ι\iota is measurable with respect to B(RdN)⊗B(Rd)\mathcal{B}(\mathbb{R}^{dN})\otimes\mathcal{B}(\mathbb{R}^{d}) and B(RdN+d)\mathcal{B}(\mathbb{R}^{dN+d}), so by claim 4 of Borel Measurability and Bounded Integration on a Metric Space the compositions with ι\iota of all these functions are measurable for the product σ\sigma-algebra. By Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §projections and (1), Δ^(ι(x,y))=Δ(x,y)\hat{\Delta}(\iota(x,y))=\Delta(x,y), where Δ(x,y)=ax(y)−a(y)\Delta(x,y)=a_{x}(y)-a(y). Hence the functions

F=∣Δ∣,Δ2=F2,G0(x,y)=1Bc(y)F(x,y),G1(x,y)=1Bc(y)ax(y),G2(x,y)=1Bc(y)a(y)F=|\Delta|,\qquad\Delta^{2}=F^{2},\qquad G_{0}(x,y)=\mathbf{1}_{B^{c}}(y)F(x,y),\qquad G_{1}(x,y)=\mathbf{1}_{B^{c}}(y)a_{x}(y),\qquad G_{2}(x,y)=\mathbf{1}_{B^{c}}(y)a(y)

are nonnegative and measurable with respect to B(RdN)⊗B(Rd)\mathcal{B}(\mathbb{R}^{dN})\otimes\mathcal{B}(\mathbb{R}^{d}); this proves the first assertion. By the Tonelli statement applied to FF, the function x↦∫F(x,y) λd(dy)x\mapsto\int F(x,y)\,\lambda_{d}(dy) is measurable, the function E(y)=∫F(x,y) Q(dx)E(y)=\int F(x,y)\,Q(dx) is measurable, and

T:=∫RdN(∫RdF(x,y) λd(dy))Q(dx)=∫RdE dλdin [0,∞].(2)T:=\int_{\mathbb{R}^{dN}}\Bigl(\int_{\mathbb{R}^{d}}F(x,y)\,\lambda_{d}(dy)\Bigr)Q(dx)=\int_{\mathbb{R}^{d}}E\,d\lambda_{d}\qquad\text{in }[0,\infty].\tag{2}

Since axa_{x} and aa are nonnegative, F(x,y)≤ax(y)+a(y)F(x,y)\le a_{x}(y)+a(y), so ∫F(x,y) λd(dy)≤1+1=2\int F(x,y)\,\lambda_{d}(dy)\le1+1=2; thus the function x↦∫F(x,y) λd(dy)x\mapsto\int F(x,y)\,\lambda_{d}(dy) takes values in [0,2][0,2] and is a Borel real function (Measure Spaces and the Lebesgue Integral: Standing Notation §measurable), proving the second assertion.

Step 2 (Pointwise variance). Fix y∈Rdy\in\mathbb{R}^{d} and let φy(x′)=ηε(y−x′)\varphi_{y}(x')=\eta_{\varepsilon}(y-x'). By Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §density and Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §kernel, φy\varphi_{y} is Borel with 0≤φy≤cεS0\le\varphi_{y}\le c_{\varepsilon}S, so it is bounded, and ∫φy dμ=a(y)\int\varphi_{y}\,d\mu=a(y); by (1), ∫φy dμxN=ax(y)\int\varphi_{y}\,d\mu^{N}_{x}=a_{x}(y) for every xx (Basic Properties of Empirical Measures: Values, Integrals, Push-Forwards, Second Moment, and Lipschitz Dependence on the Configuration §integral). Apply Mean-Square Deviation of the Empirical Average of a Bounded Borel Function under a Tensor Power with q=dq=d, ρ=μ\rho=\mu and φ=φy\varphi=\varphi_{y}: its number written aa there is a(y)a(y), its function gg is x↦ax(y)x\mapsto a_{x}(y) by Mean-Square Deviation of the Empirical Average of a Bounded Borel Function under a Tensor Power §average, and Mean-Square Deviation of the Empirical Average of a Bounded Borel Function under a Tensor Power §variance gives

V(y):=∫RdNΔ(x,y)2 Q(dx)≤1N∫Rdφy2 dμ.V(y):=\int_{\mathbb{R}^{dN}}\Delta(x,y)^{2}\,Q(dx)\le\frac{1}{N}\int_{\mathbb{R}^{d}}\varphi_{y}^{2}\,d\mu .

Multiplying 0≤φy≤cεS0\le\varphi_{y}\le c_{\varepsilon}S by φy≥0\varphi_{y}\ge0 gives φy2≤cεS φy\varphi_{y}^{2}\le c_{\varepsilon}S\,\varphi_{y} pointwise, so ∫φy2 dμ≤cεS a(y)\int\varphi_{y}^{2}\,d\mu\le c_{\varepsilon}S\,a(y) and

V(y)≤v a(y)for every y∈Rd.(3)V(y)\le v\,a(y)\qquad\text{for every }y\in\mathbb{R}^{d}.\tag{3}

Step 3 (Inside the ball). Let θ=v c−1\theta=\sqrt{v\,c^{-1}}; then 0≤θ0\le\theta and θ2=v c−1>0\theta^{2}=v\,c^{-1}>0, so 0<θ0<\theta. For all x,yx,y, 0≤(F(x,y)−θ)2=Δ(x,y)2−2θF(x,y)+θ20\le(F(x,y)-\theta)^{2}=\Delta(x,y)^{2}-2\theta F(x,y)+\theta^{2}, hence

F(x,y)≤θ2+(2θ)−1Δ(x,y)2.F(x,y)\le\frac{\theta}{2}+(2\theta)^{-1}\Delta(x,y)^{2}.

Integrating in xx against the probability measure QQ, the constant θ2\frac{\theta}{2} having integral θ2Q(RdN)=θ2\frac{\theta}{2}Q(\mathbb{R}^{dN})=\frac{\theta}{2} by The Integral of an Indicator Function is the Measure of the Set, and using (3),

E(y)≤θ2+(2θ)−1V(y)≤θ2+(2θ)−1v a(y)(y∈Rd).E(y)\le\frac{\theta}{2}+(2\theta)^{-1}V(y)\le\frac{\theta}{2}+(2\theta)^{-1}v\,a(y)\qquad(y\in\mathbb{R}^{d}).

Multiplying by 1B(y)\mathbf{1}_{B}(y) and integrating in yy, with ∫1B dλd=λd(B)=c\int\mathbf{1}_{B}\,d\lambda_{d}=\lambda_{d}(B)=c (The Integral of an Indicator Function is the Measure of the Set) and ∫1Ba dλd≤∫a dλd=1\int\mathbf{1}_{B}a\,d\lambda_{d}\le\int a\,d\lambda_{d}=1,

∫Rd1B E dλd≤θc2+v θ−12.\int_{\mathbb{R}^{d}}\mathbf{1}_{B}\,E\,d\lambda_{d}\le\frac{\theta c}{2}+\frac{v\,\theta^{-1}}{2}.

Both θc\theta c and v θ−1v\,\theta^{-1} are nonnegative with square θ2c2=v c=v2θ−2\theta^{2}c^{2}=v\,c=v^{2}\theta^{-2}, so both equal v c\sqrt{v\,c} by the uniqueness in Existence and Uniqueness of the Nonnegative Square Root. Since v c=κdRdS cεN−1v\,c=\kappa_{d}R^{d}S\,c_{\varepsilon}N^{-1},

∫Rd1B E dλd≤κd Rd S (ε−1)d N−1.(4)\int_{\mathbb{R}^{d}}\mathbf{1}_{B}\,E\,d\lambda_{d}\le\sqrt{\kappa_{d}\,R^{d}\,S\,(\varepsilon^{-1})^{d}\,N^{-1}} .\tag{4}

Step 4 (Outside the ball). Let H^(w)=1Bc(pr2(w)) ηε(pr2(w)−pr1(w))\hat{H}(w)=\mathbf{1}_{B^{c}}(\mathrm{pr}_{2}(w))\,\eta_{\varepsilon}(\mathrm{pr}_{2}(w)-\mathrm{pr}_{1}(w)) for w∈Rd+dw\in\mathbb{R}^{d+d}; as in Step 1, H^\hat H is Borel, and H=H^∘ιd,dH=\hat{H}\circ\iota^{d,d}, H(x′,y)=1Bc(y)ηε(y−x′)H(x',y)=\mathbf{1}_{B^{c}}(y)\eta_{\varepsilon}(y-x'), is nonnegative and measurable for B(Rd)⊗B(Rd)\mathcal{B}(\mathbb{R}^{d})\otimes\mathcal{B}(\mathbb{R}^{d}). Let τ(x′)=∫H(x′,y) λd(dy)\tau(x')=\int H(x',y)\,\lambda_{d}(dy). The Tonelli statement for (μ,λd)(\mu,\lambda_{d}) and HH shows that τ\tau is Borel and, since ∫H(x′,y) μ(dx′)=1Bc(y)a(y)\int H(x',y)\,\mu(dx')=\mathbf{1}_{B^{c}}(y)a(y) by the multiple rule,

∫Rd1Bca dλd=∫Rdτ dμ.(5)\int_{\mathbb{R}^{d}}\mathbf{1}_{B^{c}}a\,d\lambda_{d}=\int_{\mathbb{R}^{d}}\tau\,d\mu .\tag{5}

Since H(x′,y)≤ηε(y−x′)H(x',y)\le\eta_{\varepsilon}(y-x'), Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §kernel gives τ(x′)≤1\tau(x')\le1. Let A={x′∈Rd:(R−1)2≤∥x′∥2}A=\{x'\in\mathbb{R}^{d}:(R-1)^{2}\le\lVert x'\rVert^{2}\}. If x′∉Ax'\notin A, then ∥x′∥2<(R−1)2\lVert x'\rVert^{2}<(R-1)^{2} with 0<R−10<R-1, so ∥x′∥<R−1\lVert x'\rVert<R-1; for every y∈Bcy\in B^{c} the triangle inequality gives ∥y−x′∥≥∥y∥−∥x′∥>R−(R−1)=1≥ε\lVert y-x'\rVert\ge\lVert y\rVert-\lVert x'\rVert>R-(R-1)=1\ge\varepsilon, so ηε(y−x′)=0\eta_{\varepsilon}(y-x')=0, ηε\eta_{\varepsilon} being a mollifier kernel of radius ε\varepsilon (Mollifying a Probability Measure on Euclidean Space: Kernel Bounds, the Translation Estimate, the Mollified Density and Its Cost §kernel and condition 3 of Mollifier Kernel of Radius δ\delta on Rn\mathbb{R}^n); thus H(x′,⋅)=0⋅1RdH(x',\cdot)=0\cdot\mathbf{1}_{\mathbb{R}^{d}} and τ(x′)=0\tau(x')=0. Hence 0≤τ≤1A0\le\tau\le\mathbf{1}_{A} pointwise. By The Lebesgue Integral and Null Sets: Almost-Everywhere Comparison, Markov's Inequality, and Dominated Convergence Almost Everywhere §markov, applied on (Rd,B(Rd),μ)(\mathbb{R}^{d},\mathcal{B}(\mathbb{R}^{d}),\mu) to the nonnegative Borel function x′↦∥x′∥2x'\mapsto\lVert x'\rVert^{2} (Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §functions) and the positive number t=(R−1)2t=(R-1)^{2}, the set AA is Borel and (R−1)2μ(A)≤∫∥x′∥2 μ(dx′)=M2(μ)(R-1)^{2}\mu(A)\le\int\lVert x'\rVert^{2}\,\mu(dx')=M_{2}(\mu), a real number as μ∈P2(Rd)\mu\in\mathcal{P}_{2}(\mathbb{R}^{d}) (The Second Moment of a Probability Measure on Euclidean Space and the Probability Measures with Finite Second Moment §space). With The Integral of an Indicator Function is the Measure of the Set,

∫Rdτ dμ≤μ(A)≤M2(μ)((R−1)2)−1.(6)\int_{\mathbb{R}^{d}}\tau\,d\mu\le\mu(A)\le M_{2}(\mu)\bigl((R-1)^{2}\bigr)^{-1}.\tag{6}

Now fix x∈RdNx\in\mathbb{R}^{dN}. By (1), G1(x,⋅)=∑k=1NN−1H(pk(x),⋅)G_{1}(x,\cdot)=\sum_{k=1}^{N}N^{-1}H(\mathfrak{p}_{k}(x),\cdot), a linear combination of nonnegative Borel functions with finite integrals τ(pk(x))\tau(\mathfrak{p}_{k}(x)), hence of integrable functions; by Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear, ∫G1(x,y) λd(dy)=∑k=1NN−1τ(pk(x))\int G_{1}(x,y)\,\lambda_{d}(dy)=\sum_{k=1}^{N}N^{-1}\tau(\mathfrak{p}_{k}(x)). The functions τ∘pk\tau\circ\mathfrak{p}_{k} are Borel with values in [0,1][0,1]; by Tensor Powers and One-Particle Marginals: Particle Laws, Product Integrals, Push-Forwards, Moments, Product Maps and Diagonal Shifts §particle-laws, (pk)#Q=μ(\mathfrak{p}_{k})_{\#}Q=\mu, so the change-of-variables formula of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward gives ∫τ∘pk dQ=∫τ dμ\int\tau\circ\mathfrak{p}_{k}\,dQ=\int\tau\,d\mu, and Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear with Step 0 gives

∫RdN(∫RdG1(x,y) λd(dy))Q(dx)=∑k=1NN−1∫Rdτ dμ=∫Rdτ dμ.\int_{\mathbb{R}^{dN}}\Bigl(\int_{\mathbb{R}^{d}}G_{1}(x,y)\,\lambda_{d}(dy)\Bigr)Q(dx)=\sum_{k=1}^{N}N^{-1}\int_{\mathbb{R}^{d}}\tau\,d\mu=\int_{\mathbb{R}^{d}}\tau\,d\mu .

Also ∫G2(x,y) λd(dy)=∫1Bca dλd\int G_{2}(x,y)\,\lambda_{d}(dy)=\int\mathbf{1}_{B^{c}}a\,d\lambda_{d} does not depend on xx, so by (5) its integral against the probability measure QQ is ∫τ dμ\int\tau\,d\mu as well. Since G0≤G1+G2G_{0}\le G_{1}+G_{2}, the multiple rule (1Bc(y)E(y)=∫G0(x,y) Q(dx)\mathbf{1}_{B^{c}}(y)E(y)=\int G_{0}(x,y)\,Q(dx)), the Tonelli statement for G0G_{0}, monotonicity and additivity give, with (6),

∫Rd1Bc E dλd=∫RdN(∫RdG0 dλd)dQ≤∫RdN(∫Rd(G1+G2) dλd)dQ=2∫Rdτ dμ≤2 M2(μ)((R−1)2)−1.(7)\int_{\mathbb{R}^{d}}\mathbf{1}_{B^{c}}\,E\,d\lambda_{d}=\int_{\mathbb{R}^{dN}}\Bigl(\int_{\mathbb{R}^{d}}G_{0}\,d\lambda_{d}\Bigr)dQ\le\int_{\mathbb{R}^{dN}}\Bigl(\int_{\mathbb{R}^{d}}(G_{1}+G_{2})\,d\lambda_{d}\Bigr)dQ=2\int_{\mathbb{R}^{d}}\tau\,d\mu\le2\,M_{2}(\mu)\bigl((R-1)^{2}\bigr)^{-1}.\tag{7}

Step 5 (Conclusion). Pointwise E=1BE+1BcEE=\mathbf{1}_{B}E+\mathbf{1}_{B^{c}}E, so by (2), additivity, (4) and (7),

T=∫Rd1BE dλd+∫Rd1BcE dλd≤κd Rd S (ε−1)d N−1+2 M2(μ)((R−1)2)−1,T=\int_{\mathbb{R}^{d}}\mathbf{1}_{B}E\,d\lambda_{d}+\int_{\mathbb{R}^{d}}\mathbf{1}_{B^{c}}E\,d\lambda_{d}\le\sqrt{\kappa_{d}\,R^{d}\,S\,(\varepsilon^{-1})^{d}\,N^{-1}}+2\,M_{2}(\mu)\bigl((R-1)^{2}\bigr)^{-1},

which is the asserted bound.

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