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Berry–Esseen bound for a finite independent array

Statement

Assume the Axiom of Choice. Let X1,…,Xn be independent, finite-support real random variables with EXi=0 and total variance σ2=∑iEXi2>0. If S=∑iXi and Φ is the standard-normal CDF, then sup⁡z∈R∣Pr⁡{S/σ≤z}−Φ(z)∣≤1088 ∑iE∣Xi∣3σ3.

Facts & Assumptions

Given: The finite independent array, its mean and variance hypotheses, and the Axiom of Choice.

[A1]

The Axiom of Choice and Standard normal and normal laws: assume AC, and let G have density φ(x)=(2π)−1/2e−x2/2 and total mass one.

[F1]

The exponential function is smooth and (exp⁡)′=exp⁡, The exponential dominates every fixed nonnegative integer power at +∞, and The Gaussian integral ∫−∞∞e−x2 dx=π: φ′(x)=−xφ(x), Gaussian tails vanish at infinity, and the Gaussian integral is finite with the stated normalization.

[F3]

The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a): on a closed interval, a differentiable function whose derivative is integrable has endpoint difference equal to the derivative's integral; apply it separately on each smooth piece of f′ split at the two breakpoints of h.

Proof

1.1givenalgebra

Divide each summand by σ, so it suffices to consider independent mean-zero variables with total variance one and β:=∑iE∣Xi∣3. A zero-variance summand is zero almost surely and may be removed. For r>0, let δm(r) be the supremum of {0} together with the normal-CDF errors sup⁡z∣Pr⁡{∑iXi≤z}−Φ(z) over all m-term finite-support arrays with total variance one and third-moment sum at most r3. This convention also defines δm(r)=0 when the class of arrays is empty.

1.2givenalgebra

If some summand has variance greater than 1/2, the needed Lyapunov inequality follows locally as follows. Put A=∣Xi∣ and m3=EA3; then m3>0. For U=A/m31/3, the pointwise identity 1+2U3−3U2=(U−1)2(2U+1)≥0 gives EA2/m32/3≤1, so E∣Xi∣3≥(EXi2)3/2. Therefore β≥(EXi2)3/2>1/(22)>1/3. Since any two CDF values differ by at most one, the bound δm(r)≤1088r3 holds in this case.

1.3A1F1F2given

It remains to prove the induction step when each summand variance is at most 1/2. Fix a threshold a and ϵ>0, and let h equal 1 on (−∞,a], decrease linearly to 0 on [a,a+ϵ], and equal 0 afterward. Define f(x)=ex2/2∫−∞xe−t2/2(h(t)−Eh(G)) dt, where G has the standard-normal law. On any finite interval, [F2] differentiates the integral term and the product rule differentiates the integrating factor, giving f′(x)−xf(x)=h(x)−Eh(G). The total integral of the integrand is zero, so its upper-tail form also holds.

2.1F1F2F3step 1.3

For x>0, the upper-tail formula and 0≤h≤1 give ∣f(x)∣≤ex2/2∫x∞e−t2/2dt=∫0∞e−xs−s2/2ds≤min⁡(2,1/x). For x≤0 the lower-tail formula gives the same bounds. Thus ∣xf(x)∣≤1 and the differential equation gives ∣f′(x)∣≤2. Away from the two breakpoints of the piecewise-linear h, differentiating the Stein equation gives f′′=f+xf′+h′, so ∣f′′(x)∣≤2+2∣x∣+ϵ−11[a,a+ϵ](x). On any finite segment, split at those breakpoints and apply [F3] on each smooth subinterval to the function f′; it is differentiable there, its derivative f′′ is continuous up to the one-sided endpoints, and hence integrable. Continuity of f′ lets the increments add across the breakpoints.

3.1A1F1step 2.1giveninductionalgebra

Integrating the last bound along the segment from x to x+y (and using ∣f′∣≤2 when ∣y∣>1) yields ∣f′(x+y)−f′(x)∣≤4∣y∣(1+∣x∣+ϵ−1∫011[a,a+ϵ](x+sy)ds). For the sum S−i omitting term i, its variance is at least 1/2. After dividing by its standard deviation σ−i≥1/2, its third-moment sum is at most 8r3<8r3=(2r)3, so the induction definition bounds its CDF error by δm−1(2r). Comparing the two endpoints of any interval of length ϵ with a normal interval, whose density is bounded by one, gives Pr⁡{S−i+sy∈[a,a+ϵ]}≤2ϵ+2δm−1(2r). Finally, (E∣S−i∣)2≤ES−i2=Var⁡(S−i)≤1, because E(∣S−i∣−E∣S−i∣)2≥0. Taking expectations in the increment bound therefore gives E∣f′(S−i+y)−f′(S−i)∣≤16∣y∣(1+δm−1(2r)/ϵ).

3.2A1F1F2step 1.3step 2.1algebra

Integrating by parts on [−A,A] using [F2] gives ∫−AAf′φ=[fφ]−AA+∫−AAxfφ. The boundary term tends to zero because f is bounded by step 2.1 and φ(A)→0 by [F2]; the integrals converge since f,f′ are bounded and ∣x∣φ(x) is integrable by [F1]. Hence Ef′(G)=EGf(G). The smoothing inequalities 1(−∞,a]≤ha≤1(−∞,a+ϵ] show that Pr⁡{S≤a}−Φ(a)≤Eha(S)−Eha(G)+ϵ: the normal mass of an interval of length ϵ is at most ϵ. For the reverse difference, apply the same calculation to ha−ϵ and its corresponding Stein solution; the bounds in step 2.1 are uniform in the threshold. For either smoothing function, the Stein equation identifies the expectation difference as E[f′(S)−Sf(S)], proving the displayed uniform estimate.

4.1step 3.1step 3.2givenalgebra

For the needed moment comparison, write the finite law of A=∣Xi∣ as values aj with weights pj. For every pair j,k, aj2ak≤(2aj3+ak3)/3, since 2a3+b3−3a2b=(a−b)2(2a+b)≥0. Averaging with weights pjpk gives EXi2 E∣Xi∣≤E∣Xi∣3. Put Z=S−i. Independence and mean zero give E[Xif(S)]=E[Xi2∫01f′(Z+tXi)dt], while independence also gives E[Xi2f′(Z)]=EXi2 Ef′(Z). By step 3.1, conditioning on Xi bounds E[Xi2∫01∣f′(Z+tXi)−f′(Z)∣dt] by 8E∣Xi∣3(1+δm−1(2r)/ϵ), and the same step bounds EXi2 E∣f′(Z+Xi)−f′(Z)∣ by 16EXi2 E∣Xi∣(1+δm−1(2r)/ϵ). Decomposing at f′(Z) and using the moment comparison shows ∣E[Xif(S)]−EXi2 Ef′(S)∣≤24E∣Xi∣3(1+δm−1(2r)/ϵ)≤32E∣Xi∣3(1+δm−1(2r)/ϵ). Summing over i and using ∑iEXi2=1 bounds the difference in step 3.2 by 32r3(1+δm−1(2r)/ϵ).

5.1step 1.1step 1.2step 3.2step 4.1algebra∎

Choose ϵ=512r3. Steps 3.2 and 4.1 give δm(r)≤544r3+116δm−1(2r). Inductively, δm−1(2r)≤1088(2r)3, so the right side is at most (544+544)r3=1088r3. For one summand with variance one, Lyapunov gives r3≥β≥1, and the trivial CDF bound starts the induction. Combining with step 1.2 proves the normalized claim; undoing the variance normalization proves the Statement.

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