π After-Class Exercise Detailed Explanation: Large Sample Theory Assignment 4
1. One-step estimator
Problem: Let \(\{P_{\theta}\}_{\theta\in\Theta}\) be a model family, where \(\Theta\subset\mathbb{R}^{d}\) is an open set, and \(X_{1},...,X_{n} \stackrel{i.i.d}{\sim} P_{\theta_{0}}\). The log-likelihood function \(l_{\theta}(x)=\log p_{\theta}(x)\) satisfies the given regularity conditions. Let \(\hat{\theta}_{n}\) be an \(n\)-consistent estimator. The one-step estimator \(\delta_{n}\) satisfies the following equation:
(a) Assume the model family \(\{P_{\theta}\}_{\theta\in\mathbb{R}}\) is the Cauchy family, with probability density function \(p_{\theta}(x)= \frac{1}{\pi(1+(x-\theta)^{2})}\). Let \(X_{1},...,X_{n} \stackrel{i.i.d}{\sim} P_{\theta}\) and define \(\hat{\theta}_{n}=\text{Median}(X_{1},...,X_{n})\). Find the limiting distribution of \(\sqrt{n}(\hat{\theta}_{n}-\theta)\).
(b) Let \(\delta_{n}\) be the one-step estimator for this Cauchy family. What is its asymptotic distribution? In (a), is \(\delta_{n}\) more efficient than \(\hat{\theta}_{n}\)?
Solution (click to expand)
(a) Find the asymptotic distribution of the sample median
The sample median \(\hat{\theta}_{n}\) corresponds to the sample quantile at \(p=1/2\). According to the established asymptotic theory for sample quantiles (e.g., Theorem 5.23 in van der Vaart), if the cumulative distribution function \(F\) has a continuous and strictly positive derivative (density) \(f\) at the true population quantile \(\theta\), then the sample median is asymptotically normal:
For \(p=1/2,\) the numerator of the variance is \(1/4.\) We now compute the Cauchy density at the true median \(\theta\):
Substituting \(f(\theta)=1/\pi\) into the asymptotic variance formula:
Therefore, the limiting distribution of the sample median is:
(b) Find the asymptotic distribution of the one-step estimator and compare efficiency
According to the definition of the one-step estimator, we can rewrite it as:
We use Taylor's theorem to expand the score function \(\frac{1}{\sqrt{n}}\nabla L_{n}(\hat{\theta}_{n})\) around the true parameter \(\theta\):
where \(\tilde{\theta}\) lies between \(\hat{\theta}_{n}\) and \(\theta\). Since \(\hat{\theta}_{n}\) is \(\sqrt{n}\)-consistent, \(\tilde{\theta}\xrightarrow{P}\theta\). By the Weak Law of Large Numbers and the Lipschitz continuity of the second derivative, we have:
where \(I(\theta)=-E[\nabla^{2}l_{\theta}(X)]\) is the Fisher information. Substituting the Taylor expansion back into our estimator, we obtain:
By the Central Limit Theorem, the standardized score function \(\frac{1}{\sqrt{n}}\nabla L_{n}(\theta)\xrightarrow{d}\mathcal{N}(0,I(\theta))\). By Slutsky's theorem, the one-step estimator achieves the efficiency of the maximum likelihood estimator:
Now, we compute the Fisher information \(I(\theta)\) for the Cauchy distribution. The log-density is:
The first derivative (score function) is:
The Fisher information is the expectation of the squared score:
Let \(y=x-\theta\). Since the integrand is an even function:
We can solve this via the trigonometric substitution \(y=\tan z\), which gives \(dy=\sec^{2}z dz\) and \(1+y^{2}=\sec^{2}z\). The interval changes from \([0,\infty)\) to \([0,\pi/2)\):
Let \(u=2z\), so \(du=2dz\), and the interval becomes \([0, \pi]\):
Therefore, the asymptotic variance of the one-step estimator is \(I(\theta)^{-1}=2\).
Efficiency comparison: From part (a), the asymptotic variance of the sample median \(\hat{\theta}_{n}\) is \(\frac{\pi^{2}}{4}\approx2.467\). Since \(2<\frac{\pi^{2}}{4}\), the asymptotic variance of the one-step estimator \(\delta_{n}\) is strictly smaller than that of the initial median estimator \(\hat{\theta}_{n}\). Therefore, \(\delta_{n}\) is more efficient.
2. Unbiased estimator and U-statistic
Problem: Let \(X_{1},...,X_{n}\) be i.i.d. random variables, with finite \(\mu=\mathbb{E}(X_{1})\) and \(\overline{\mu}=\mathbb{E}(X_{1}^{-1})\). Find a U-statistic that is an unbiased estimator of \(\overline{\mu}\mu\), and derive its variance and asymptotic distribution.
Solution (click to expand)
Step 1: Construct a symmetric kernel and the U-statistic
We want to estimate \(\theta=\mu\overline{\mu}\). Consider a pair of independent observations \((X_{1},X_{2})\). Since they are independent, we have:
Thus, \(g(x_{1},x_{2})=x_{1}x_{2}^{-1}\) is an unbiased estimator of \(\theta\), but it is asymmetric. We construct a symmetric kernel of degree \(m=2\) by averaging over permutations:
Clearly, \(\mathbb{E}[h(X_{1},X_{2})]=\frac{1}{2}(\mu\overline{\mu}+\mu\overline{\mu})=\mu\overline{\mu}\). The corresponding U-statistic is:
Step 2: Derive the variance of \(U_{n}\)
According to Hoeffding's theorem, the variance of a U-statistic of degree \(m=2\) is given by:
First, we compute \(h_{1}(x_{1})=\mathbb{E}[h(X_{1},X_{2})|X_{1}=x_{1}]\):
Now we compute \(\zeta_{1}=Var(h_{1}(X_{1}))\). Let \(\sigma^{2}=Var(X_{1})\) and \(\overline{\sigma}^{2}=Var(X_{1}^{-1})\). Using the property \(Var(aX+bY)=a^{2}Var(X)+b^{2}Var(Y)+2abCov(X,Y)\):
Next, we compute \(\zeta_{2}=Var(h(X_{1},X_{2}))=\mathbb{E}[h^{2}(X_{1},X_{2})]-(\mu\overline{\mu})^{2}\):
Recall the relations between second moments and variances: \(\mathbb{E}[X_{1}^{2}]=\sigma^{2}+\mu^{2}\) and \(\mathbb{E}[X_{1}^{-2}]=\overline{\sigma}^{2}+\overline{\mu}^{2}\). Substituting these into the equation:
Substituting \(\zeta_{1}\) and \(\zeta_{2}\) back into the formula gives the exact variance:
Step 3: Derive the asymptotic distribution
According to the projection theorem for U-statistics (Hoeffding's CLT), since \(\mathbb{E}[h^{2}]<\infty\) and \(\zeta_{1}>0\), the U-statistic is asymptotically normal, driven by the first-order projection:
where the kernel degree is \(m=2\). Therefore, the asymptotic variance is \(4\zeta_{1}\):
Thus, the asymptotic distribution is:
3. Hoeffding's theorem
Problem: Let \(X_{1},...,X_{n} \stackrel{i.i.d}{\sim} P\in\mathcal{P}\) and \(\mathbb{E}_{P}h^{2}(X_{1},...,X_{m})<\infty\), then:
where \(\xi_{k}=Var_{P}(h_{k}(X_{1},...,X_{k}))\).
(a) Prove \(\frac{m^{2}}{n}\xi_{1}\le Var_{P}(U_{n})\le\frac{m}{n}\xi_{m}\)
(b) Prove \((n+1)Var_{P}(U_{n+1})\le nVar_{P}(U_{n})\)
Solution (click to expand)
(a) Prove the upper and lower bounds
According to the Hoeffding H-decomposition (ANOVA decomposition) for U-statistics, we can rewrite the variance of \(U_{n}\) in terms of the projection variances \(\eta_{j}\) (the variances of the \(j\)-th order orthogonal projection kernels):
By definition, for all \(j=1,...,m\), \(\eta_{j}\ge0\). The relationship between \(\xi_{k}\) and \(\eta_{j}\) is given by:
In particular, for \(k=1\), we have \(\xi_{1}=\binom{1}{1}\eta_{1}=\eta_{1}\). For \(k=m\), we have \(\xi_{m}=\sum_{j=1}^{m}\binom{m}{j}\eta_{j}\).
Lower bound: Since all terms in the variance sum are non-negative \((\eta_{j}\ge0)\), the total variance is bounded below by its first term \((j=1)\):
Upper bound: We analyze the combinatorial coefficients in the variance sum. We can rewrite them as:
Expanding the term in brackets:
Since \(m\le n\), for any \(i\ge0\), we have \(nn-in\le mn-im\), which implies \(\frac{m-i}{n-i}\le\frac{m}{n}\). Therefore, the product is bounded by:
Substituting this inequality back into the variance formula, we obtain:
Since \(\xi_{m}=\sum_{j=1}^{m}\binom{m}{j}\eta_{j}\), we conclude:
(b) Prove the sample size recursion inequality
Using the variance formula from the H-decomposition, we write the scaled variances for sample sizes \(n\) and \(n+1\):
To prove the inequality, it suffices to show that the coefficient of each \(\eta_{j}\) is non-increasing when the sample size increases from \(n\) to \(n+1\). We compare the terms in brackets. For size \(n+1\):
We can factor out \((n-j+1)\) from the numerator:
Since for all terms in the sum \(j\ge1\), we clearly have \(n-j+1\le n\). Therefore:
Because \(\binom{m}{j}^{2}\eta_{j}\ge0\) for all \(j\), multiplying this non-negative constant to both sides of the inequality preserves the direction. Summing over all \(j=1,...,m\) yields:
This is precisely:
Exercise 4: U-statistics and V-statistics
Problem: Let \(X_1, X_2, \dots\) be a sequence of i.i.d. random variables, and let \(h\) be a symmetric kernel function satisfying \(0 < E[h^2(X_1, X_2)] < \infty\) and \(E[h^2(X_1, X_1)] < \infty\). Define \(V_n\) as:
(a) Use the central limit theorem for U-statistics to prove that \(V_n\) is asymptotically normal.
(b) Can \(V_n\) be written as a U-statistic? Why?
(c) Now assume \(E X_1 = 0\) and \(E X_1^4 < \infty\). Take the kernel \(h(x, y) = xy\). Find the asymptotic relative efficiency (ARE) of \(V_n\) relative to the U-statistic \(U_n := \frac{2}{n(n-1)} \sum_{1 \le i < j \le n} X_i X_j\), i.e., \(\frac{Avar(U_n)}{Avar(V_n)}\).
Solution (click to expand)
(a) Prove the asymptotic normality of \(V_n\)
Let \(\theta = E[h(X_1, X_2)]\) be the expectation of the kernel for independent observations. The corresponding U-statistic is:
We can decompose the V-statistic into the U-statistic part (off-diagonal terms) and the diagonal part:
To analyze its asymptotic distribution, we scale the centered V-statistic by \(\sqrt{n}\):
Let \(\mu_D = E[h(X_1, X_1)]\). By the Weak Law of Large Numbers (WLLN), \(\frac{1}{n} \sum_{i=1}^n h(X_i, X_i) \xrightarrow{p} \mu_D\). Therefore, the last term in the expression is \(\frac{1}{n} (\frac{1}{n} \sum h(X_i, X_i)) = O_p(n^{-1})\), which is \(o_p(1)\). Meanwhile, the scaling factor \((1 - 1/n) \rightarrow 1\).
By Slutsky's theorem, the scaled difference of the V-statistic converges to that of the U-statistic:
According to the central limit theorem for U-statistics, \(\sqrt{n}(U_n - \theta) \xrightarrow{d} \mathcal{N}(0, 4\zeta_1)\). Hence \(V_n\) has the same asymptotic normal distribution:
(b) Can \(V_n\) be written as a U-statistic?
No. By definition, a U-statistic \(U_n\) of size \(n\) must be an unbiased estimator of its population parameter \(\theta\), i.e., \(E[U_n] = \theta\) for all \(n \ge m\). Compute the expectation of \(V_n\):
Since \(E[V_n]\) explicitly depends on the sample size \(n\) (unless \(\theta = \mu_D\), which is not generally true), \(V_n\) is a biased estimator and cannot be a U-statistic.
(c) Compute the asymptotic relative efficiency (ARE)
Since \(E X_1 = 0\) and \(h(x, y) = xy\), we compute \(\theta\) and the projection variance \(\zeta_1\):
The projection function is:
Because \(h_1(x_1) \equiv 0\), we have \(\zeta_1 = Var(h_1(X_1)) = 0\). This means \(U_n\) is a degenerate U-statistic, and the standard \(\sqrt{n}\) scaling yields a limit of 0. We need to use a scaling factor of \(n\).
Analysis of \(n V_n\):
By the CLT, \(\sqrt{n}\bar{X}_n \xrightarrow{d} \mathcal{N}(0, \sigma^2)\). By the Continuous Mapping Theorem (CMT):
Its asymptotic variance is \(Var(\sigma^2 \chi_1^2) = \sigma^4 Var(\chi_1^2) = \sigma^4 \cdot 2 = 2\sigma^4\).
Analysis of \(n U_n\):
Its asymptotic variance is \(Var(\sigma^2(\chi_1^2 - 1)) = \sigma^4 Var(\chi_1^2) = 2\sigma^4\).
Hence, the ARE is:
Exercise 5: Divide and Conquered U-statistics for big data
Problem: Let \(U_N\) be a U-statistic with kernel \(h(x_1, \dots, x_m)\). Assume \(\theta = E[h(X_1, \dots, X_m)]\) and \(E[|h|] < \infty\). Define \(h_1(x_1) = E[h(X_1, X_2, \dots, X_m) | X_1 = x_1]\) and assume \(\zeta_1 = Var(h_1(X_1)) > 0\). Suppose the total sample size is \(N = nK\), and the data are partitioned into \(K\) non-overlapping subsets \(D_k\) (each of size \(n\)). Let \(U_{kn}\) be the U-statistic based on the \(k\)-th subset \(D_k\). Define \(AU_N = K^{-1} \sum_{k=1}^K U_{kn}\). Prove: if \(K = o(N)\), then \(\sqrt{N}(AU_N - \theta) \xrightarrow{d} \mathcal{N}(0, m^2\zeta_1)\).
Solution (click to expand)
Proof:
We need to show that \(\sqrt{N}(AU_N - \theta) \xrightarrow{d} \mathcal{N}(0, m^2\zeta_1)\). We rewrite the scaled averaged U-statistic as a sum of independent random variables. Since \(N = nK\), we have:
For a given total sample size \(N\) (hence \(n\) and \(K\) fixed), define \(Z_{N,k} = \sqrt{\frac{n}{K}} (U_{kn} - \theta)\). Because the \(K\) subsets are non-overlapping, \(\{Z_{N,k}\}_{k=1}^K\) forms a triangular array of row-wise independent random variables. We will use the Lindeberg-Feller central limit theorem.
Step 1: Convergence of the row sum variance
Let \(S_N = \sum_{k=1}^K Z_{N,k}\). Since the \(Z_{N,k}\) are i.i.d. for fixed \(N\):
From standard U-statistic theory, for a sample of size \(n\), \(n Var(U_{kn}) \rightarrow m^2 \zeta_1\) (as \(n \rightarrow \infty\)). Because \(K = o(N)\), i.e., \(K/N \rightarrow 0\), this implies \(n = N/K \rightarrow \infty\). Therefore:
Step 2: Verification of the Lindeberg condition
We need to show that for any \(\epsilon > 0\):
Since the \(Z_{N,k}\) are identically distributed, the sum simplifies to:
Let \(W_n = \sqrt{n}(U_{1n} - \theta)\). The above expectation becomes \(E[W_n^2 I(|W_n| > \epsilon \sqrt{K})]\). By the CLT for regular U-statistics, \(W_n \xrightarrow{d} \mathcal{N}(0, m^2\zeta_1)\). Moreover, we know \(E[W_n^2] = n Var(U_{1n}) \rightarrow m^2 \zeta_1\). Convergence in distribution together with convergence of second moments implies that \(\{W_n^2\}\) is uniformly integrable (UI). For any uniformly integrable sequence, if the truncation threshold tends to infinity, the truncated expectation tends to 0. Since \(K \rightarrow \infty\), the threshold \(\epsilon \sqrt{K} \rightarrow \infty\). Hence:
This satisfies the Lindeberg condition.
Step 3: Conclusion
Since the Lindeberg condition holds and the variance of the row sums converges to \(m^2\zeta_1\), by the Lindeberg-Feller central limit theorem:
The proof is complete. \(\square\)