← Big Ideas of Statistics Graduate
Graduate edition · for PhD students in statistics

The big ideas of statistics, with the fine print

Twelve results every statistics PhD student should be able to state, sketch a proof of, and say where they fail. Each one has a simulation aimed at the edges of the theorem: small samples, boundaries, high dimensions and misspecification. That is where theory and practice part ways.

How to read this

Each idea has five parts. The statement gives the theorem in its usual form. Why it's true is a proof sketch you should be able to reconstruct. Where it breaks covers the failure modes that show up in qualifying exams and in practice. Key references lists the primary literature. The lab lets you test the claim yourself.

Notation: $\rightsquigarrow$ is weak convergence, $\mathbb P_n$ is the empirical measure, $I(\theta)$ is Fisher information per observation, and $a \lesssim b$ means $a \le Cb$ for a universal constant $C$.

Part I

Likelihood & asymptotics

Classical theory rests on one approximation: near the truth, the log-likelihood is a quadratic. Almost every textbook asymptotic result follows from it, and each one fails when the quadratic approximation fails.

01

Fisher information & the asymptotic trinity

The curvature of the log-likelihood bounds how precise any estimator can be. The three standard ways of turning that curvature into an interval are not equally honest.

Statement

In a regular parametric family, the score $U_n(\theta)=\partial_\theta \ell_n(\theta)$ has mean zero and variance $nI(\theta)$. For any unbiased $T$, the Cramér–Rao bound gives $\operatorname{Var}_\theta T \ge \{nI(\theta)\}^{-1}$, and the MLE attains it asymptotically:

$$\sqrt{n}\,(\hat\theta_n-\theta)\rightsquigarrow N\!\big(0,\ I(\theta)^{-1}\big),\qquad I(\theta)=\mathbb E_\theta\!\left[-\partial_\theta^2\log f(X;\theta)\right].$$

The modern form of "efficiency" doesn't need unbiasedness. Le Cam's local asymptotic normality (LAN) says that

$$\ell_n(\theta+h/\sqrt n)-\ell_n(\theta)=h\Delta_n-\tfrac12 h^2 I(\theta)+o_p(1),\qquad \Delta_n\rightsquigarrow N(0,I(\theta)).$$

Hájek's convolution theorem then shows that every regular estimator's limit is $N(0,I^{-1})$ convolved with independent noise. Hodges' superefficient estimator shows why the regularity requirement is needed: it beats $I^{-1}$ at a single point and pays for it nearby.

Why it's true

Expand $0=U_n(\hat\theta)\approx U_n(\theta)+(\hat\theta-\theta)\,\partial_\theta U_n(\theta)$. The CLT gives $U_n/\sqrt n\rightsquigarrow N(0,I)$, the LLN gives $-\partial_\theta U_n/n\to I$, and Slutsky finishes the argument. The Wald, score and likelihood-ratio statistics are three readings of the same quadratic. They agree to first order and differ at $O(n^{-1/2})$.

For a binomial proportion, the Wald test gives $\hat p\pm z\sqrt{\hat p(1-\hat p)/n}$. Inverting the score test gives the Wilson interval, which evaluates the variance at the null value rather than at $\hat p$:

$$\frac{\hat p+\frac{z^2}{2n}}{1+\frac{z^2}{n}}\ \pm\ \frac{z}{1+\frac{z^2}{n}}\sqrt{\frac{\hat p(1-\hat p)}{n}+\frac{z^2}{4n^2}}$$

Where it breaks

(i) Discreteness. Wald coverage oscillates with $(n,p)$ and collapses near $0$ and $1$, even for large $n$. The lab computes it exactly. (ii) The support depends on $\theta$, as in $\mathrm{Unif}(0,\theta)$, so the rate is $n$, not $\sqrt n$ (see idea 8). (iii) The number of parameters grows with $n$. In the Neyman–Scott problem the MLE of $\sigma^2$ converges to $\sigma^2/2$. (iv) Boundaries and non-identifiability (see idea 2).

Key references

Fisher (1922, 1925); Rao (1945); Cramér (1946); Neyman & Scott (1948); Le Cam (1953, 1960); Hájek (1970, 1972); Agresti & Coull (1998); Brown, Cai & DasGupta, Statistical Science (2001).

Lab · Exact coverage of binomial intervals
Wald Wilson (score) Agresti–Coull Nominal
Coverage is computed exactly as $C(p)=\sum_x \binom nx p^x(1-p)^{n-x}\,\mathbf 1\{p\in \mathrm{CI}(x)\}$. No simulation is involved. Increase $n$: the Wald interval still has "unlucky" values of $p$ well inside $[0.1, 0.9]$.
02

Wilks' theorem, and what happens at the boundary

The likelihood ratio is asymptotically χ² only when the truth is in the interior. On a boundary, the limit becomes a squared distance to a cone.

Statement

Let $\Theta_0\subset\Theta\subseteq\mathbb R^k$ be smooth with $\dim\Theta_0=k_0$, and let $\theta_0$ be an interior point. Under regularity, $\Lambda_n=2\{\sup_\Theta\ell_n-\sup_{\Theta_0}\ell_n\}\rightsquigarrow\chi^2_{k-k_0}$. In general (Chernoff, 1954), the limit is

$$\Lambda_n\rightsquigarrow \inf_{t\in C_{\Theta_0}}\|Z-t\|^2_{I}-\inf_{t\in C_{\Theta}}\|Z-t\|^2_{I},\qquad Z\sim N\!\big(0,I(\theta_0)^{-1}\big),$$

where $C_\Theta$ and $C_{\Theta_0}$ are the tangent cones at $\theta_0$ and $\|v\|_I^2=v^\top I(\theta_0)v$. At an interior point the cones are linear subspaces, and the difference of squared projection distances is $\chi^2_{k-k_0}$.

Why it's true

By LAN, the log-likelihood ratio is locally $h^\top\Delta_n-\frac12 h^\top I h$. Maximizing a concave quadratic over a cone means projecting the Gaussian $I^{-1}\Delta_n$ onto that cone. For $X_i\sim N(\mu,1)$ with $\mu\ge0$ and $H_0:\mu=0$, the cone is a half-line, so $\Lambda_n = n\max(\bar X,0)^2$ and

$$\Lambda_n\ \stackrel{d}{=}\ \tfrac12\chi^2_0+\tfrac12\chi^2_1 .$$

This is exactly the situation when testing a variance component $\sigma_b^2=0$ in a mixed model. Comparing against $\chi^2_1$ halves the true size: the test is conservative, and power is lost. In finite samples the Bartlett correction $\Lambda_n/\{1+b/n\}$ reduces the $\chi^2$ approximation error from $O(n^{-1})$ to $O(n^{-2})$.

Where it breaks

Boundary parameters (variance components, one-sided constraints) give chi-bar-squared mixtures. Testing the number of mixture components is worse still: the parameter isn't identified under $H_0$, and the LR statistic diverges (Hartigan, 1985). Small $n$ in skewed models shifts the null distribution, as the "regular" lab setting with $n=2$ shows.

Key references

Wilks (1938); Bartlett (1937); Chernoff (1954); Self & Liang, JASA (1987); Stram & Lee (1994); Hartigan (1985); Drton (2009), "Likelihood ratio tests and singularities."

Lab · Null distribution of the LR statistic
Simulated $\Lambda_n$ (density, excluding any atom at 0) $\chi^2_1$ density
03

Empirical processes

The empirical distribution converges uniformly, at a rate that doesn't depend on $F$, and the $\sqrt n$-scaled fluctuation is a Brownian bridge.

Statement

Glivenko–Cantelli: $\|F_n-F\|_\infty\to0$ almost surely. Donsker: $\sqrt n(F_n-F)\rightsquigarrow \mathbb B\circ F$ in $\ell^\infty(\mathbb R)$, where $\mathbb B$ is a Brownian bridge. For continuous $F$ the continuous mapping theorem then gives Kolmogorov's distribution-free limit. DKW, with Massart's sharp constant, gives a finite-sample band:

$$P\Big(\sup_x|F_n(x)-F(x)|>\varepsilon\Big)\le 2e^{-2n\varepsilon^2},\qquad P\big(\sqrt n D_n\le x\big)\to1-2\sum_{k\ge1}(-1)^{k-1}e^{-2k^2x^2}.$$

Why it matters

Replace half-lines $\{(-\infty,x]\}$ by a general class $\mathcal F$ and study $\|\mathbb P_n-P\|_{\mathcal F}=\sup_{f\in\mathcal F}|(\mathbb P_n-P)f|$. Uniform laws hold when $\mathcal F$ is small enough, as measured by VC dimension, covering numbers or bracketing entropy. This one idea gives consistency of M-estimators (argmax continuous mapping), the functional delta method (quantiles, bootstrap of smooth functionals), generalization bounds in learning theory, and the Donsker conditions behind semiparametric efficiency (idea 12). Chaining (Dudley's entropy integral) is the main proof technique.

Where it breaks

(i) Classes that are too rich. For continuous $P$, $\sup_{A\ \text{Borel}}|\mathbb P_n(A)-P(A)|=1$ for every $n$: take $A$ to be the sample itself. (ii) Dependence requires mixing conditions, and the limiting variance changes. (iii) If $F$ is discontinuous, the KS test is no longer distribution-free and becomes conservative. (iv) Estimated parameters: testing normality with $\hat\mu,\hat\sigma$ plugged in changes the null distribution (Lilliefors).

Key references

Glivenko (1933); Cantelli (1933); Kolmogorov (1933); Donsker (1952); Dvoretzky, Kiefer & Wolfowitz (1956); Massart (1990); Vapnik & Chervonenkis (1971); Dudley (1978); van der Vaart & Wellner, Weak Convergence and Empirical Processes (1996).

Lab · ECDF, DKW band and the Kolmogorov law
$F_n$ $F(x)=x$ 95% DKW band $D_n$ location
Distribution of $\sqrt n D_n$ across simulations
Simulated $\sqrt n D_n$ Kolmogorov density
Part II

Decisions & computation

Wald's decision theory asks which estimators can be beaten. The answer, Stein's shrinkage, led straight to hierarchical Bayes, and hierarchical Bayes required a way to compute high-dimensional integrals.

04

Stein's paradox & empirical Bayes

In three or more dimensions, shrinking toward any fixed point lowers the total squared-error risk everywhere. So the obvious estimator is inadmissible.

Statement

Let $X\sim N_p(\theta,I_p)$ with loss $\|\hat\theta-\theta\|^2$. The MLE $\hat\theta=X$ is minimax with constant risk $p$, yet for $p\ge3$ it is inadmissible (Stein, 1956). The James–Stein estimator $\hat\theta^{JS}=\big(1-\tfrac{p-2}{\|X\|^2}\big)X$ satisfies

$$R(\theta,\hat\theta^{JS})=p-(p-2)^2\,\mathbb E_\theta\!\left[\|X\|^{-2}\right]\ \lt\ p\quad\text{for all }\theta,$$

and its positive part $\hat\theta^{JS+}=(1-\tfrac{p-2}{\|X\|^2})_+X$ dominates it in turn (and is itself inadmissible). At $\theta=0$ the risk falls from $p$ to $2$.

Why it's true

Stein's lemma: $\mathbb E[(X_i-\theta_i)g(X)]=\mathbb E[\partial_i g(X)]$. Write $\hat\theta=X+g(X)$. Then $R=p+\mathbb E[\|g\|^2+2\nabla\!\cdot g]$, and SURE is an unbiased risk estimate. With $g=-(p-2)X/\|X\|^2$ we get $\nabla\!\cdot g=-(p-2)^2/\|X\|^2$. Empirical Bayes reading: if $\theta_i\stackrel{iid}{\sim}N(0,\tau^2)$, the Bayes rule is $(1-B)X$ with $B=1/(1+\tau^2)$. Since $\|X\|^2\sim(1+\tau^2)\chi^2_p$ and $\mathbb E[1/\chi^2_p]=1/(p-2)$, the factor $(p-2)/\|X\|^2$ is unbiased for $B$. James–Stein is what you get by estimating the prior from the data (Efron & Morris, 1973).

Why $p\ge3$? Brown (1971) showed that admissibility of generalized Bayes rules is equivalent to recurrence of an associated diffusion. Brownian motion is recurrent in dimensions 1 and 2 and transient in 3 or more.

Where it breaks

The improvement is in total risk. Individual coordinates, especially the extreme ones, can be made worse, which is why Efron and Morris proposed limited-translation rules. The gain disappears when $\|\theta\|^2\gg p$, that is, when you shrink toward the wrong point. Under heteroscedastic or non-Gaussian errors, you need SURE-tuned or nonparametric EB alternatives.

Key references

Stein (1956); James & Stein (1961); Baranchik (1964); Brown (1971); Efron & Morris (1973, 1975: the baseball data); Stein (1981), SURE; Robbins (1956), empirical Bayes; Efron, Large-Scale Inference (2010).

Lab · Risk of MLE vs. James–Stein
MLE (risk = p) James–Stein Positive-part JS
The risk is Monte Carlo estimated (600 draws per point) along $\theta=(\|\theta\|,0,\dots,0)$, which is enough because the risk depends on $\theta$ only through $\|\theta\|$. Set $p=3$, then $p=50$: the gain near the shrinkage target grows with dimension.
05

MCMC & optimal scaling

To sample from a density known only up to a constant, build a Markov chain that leaves it invariant. Tuning decides whether "eventually" takes seconds or centuries.

Statement

Metropolis–Hastings proposes $y\sim q(x,\cdot)$ and accepts with probability

$$\alpha(x,y)=\min\!\left\{1,\ \frac{\pi(y)\,q(y,x)}{\pi(x)\,q(x,y)}\right\},$$

which enforces detailed balance $\pi(x)P(x,y)=\pi(y)P(y,x)$, so $\pi$ is invariant. A $\pi$-irreducible, aperiodic chain satisfies the ergodic theorem. Under geometric ergodicity a Markov chain CLT also holds, with asymptotic variance $\sigma_f^2\,(1+2\sum_{k\ge1}\rho_k)$. The effective sample size is $\mathrm{ESS}=N/(1+2\sum_k\rho_k)$.

Optimal scaling

For random-walk Metropolis on product targets in dimension $d$ with proposal $N(0,\ell^2 I_d/d)$, each coordinate converges to a Langevin diffusion as $d\to\infty$. Its speed $h(\ell)=2\ell^2\Phi(-\ell\sqrt{J}/2)$ is maximized when the acceptance rate is about 0.234 (Roberts, Gelman & Gilks, 1997). Steps that are too small give high acceptance but a slow random walk. Steps that are too large almost always get rejected. The number of steps to mix scales as $O(d)$ for RWM, $O(d^{1/3})$ for MALA, and $O(d^{1/4})$ for HMC.

Where it breaks

Strong correlations and curved geometry (try the banana target) defeat isotropic proposals at any scale. Multimodality can leave a chain stuck forever in one mode while every diagnostic looks fine. Diagnostics such as rank-normalized $\hat R$ and bulk/tail ESS can show that a chain hasn't converged. They can never prove that it has.

Key references

Metropolis et al. (1953); Hastings (1970); Geman & Geman (1984); Gelfand & Smith (1990); Gelman & Rubin (1992); Geyer (1992), initial-sequence estimators; Roberts, Gelman & Gilks (1997); Neal (2011), HMC; Hoffman & Gelman (2014), NUTS; Vehtari et al. (2021).

Lab · Random-walk Metropolis
Target density Samples Last 150 steps
Trace of $x_1$
Part III

Multiplicity & selection

Classical guarantees assume the question was fixed before seeing the data. Modern practice screens thousands of hypotheses and reports the interesting ones. These two ideas show how to keep error guarantees honest when that happens.

06

The false discovery rate

At scale, controlling the chance of any error is the wrong target. Control the expected fraction of errors among the discoveries instead.

Statement

Given $m$ p-values, let $V$ be the number of false rejections and $R$ the total number of rejections. Then $\mathrm{FDR}=\mathbb E[V/(R\vee1)]$. The Benjamini–Hochberg step-up procedure rejects the hypotheses with the $\hat k$ smallest p-values, where

$$\hat k=\max\Big\{k:\ p_{(k)}\le \tfrac{qk}{m}\Big\},\qquad \mathrm{FDR}_{\mathrm{BH}}=\pi_0\,q\ \ \text{under independence.}$$

Why it's true

For each null $i$, write $\mathbf 1\{i\text{ rejected}\}/R=\sum_k \mathbf 1\{p_i\le qk/m,\ R=k\}/k$. Conditional on the other p-values, $R$ is a function of $p_i$ that is constant on the event that $i$ is rejected (the leave-one-out trick). Uniformity of $p_i$ then gives $\mathbb E[V_i/R]=q/m$, and summing over the $m_0$ nulls gives $\pi_0 q$. The same proof works under PRDS dependence (Benjamini & Yekutieli, 2001). Under arbitrary dependence, replace $q$ by $q/\sum_{i\le m}i^{-1}$.

Two-groups model. If $p_i\sim\pi_0\,\mathrm{U}(0,1)+(1-\pi_0)F_1$, BH is approximately thresholding the tail-area $\mathrm{Fdr}(t)=\pi_0t/G(t)$, where $G$ is the marginal CDF of the p-values. The local fdr, $\pi_0f_0/f$, is the posterior null probability (Efron). In the histogram lab you can see both: a flat floor at height $\pi_0$ and a spike at zero.

Where it breaks

FDR controls an average over replications. The realized FDP in a single study can be far above $q$, especially when $R$ is small. Negative or arbitrary dependence can break PRDS. FDR also doesn't transfer to selected subsets: the FDR among discoveries in your favorite pathway is not $q$. If you need finite-sample FDR control for variable selection, use knockoffs (Barber & Candès, 2015).

Key references

Benjamini & Hochberg, JRSS-B (1995); Benjamini & Yekutieli (2001); Storey (2002), adaptive $\hat\pi_0$; Efron et al. (2001), local fdr; Genovese & Wasserman (2002); Barber & Candès (2015).

Lab · Benjamini–Hochberg on m = 2,000 tests
True signal True null BH line $qk/m$ Bonferroni $q/m$
p-value histogram (density), stacked by truth
07

Inference after selection

Once you've looked at the data to choose the question, the selected estimate is biased toward the extreme, and the textbook interval no longer covers.

Statement

Let $X_i=\theta_i+\varepsilon_i$ with $\varepsilon_i\sim N(0,1)$ for $i=1,\dots,m$, and report $i^*=\arg\max_i X_i$. Then $\mathbb E[X_{i^*}-\theta_{i^*}]\gt0$. When the $\theta_i$ are equal, the bias grows like $\sqrt{2\log m}$, and $X_{i^*}\pm1.96$ undercovers badly. There are four principled responses:

(i) Sample splitting. Select on one half of the data and infer on the other. It's valid, and you pay in power. (ii) Conditional (selective) inference. Condition on the selection event. For polyhedral events (lasso, marginal screening), $\eta^\top y$ given selection is a truncated Gaussian (Lee et al., 2016; Fithian, Sun & Taylor, 2014). (iii) Simultaneous inference. Cover every model you might have selected (PoSI; Berk et al., 2013). (iv) Bayes. If the prior is correct, the posterior is unaffected by data-dependent selection (Dawid, 1994). Tweedie's formula estimates the needed shrinkage from the marginal density alone:

$$\mathbb E[\theta\mid X=x]=x+\sigma^2\,\frac{d}{dx}\log f(x),\qquad f=\text{marginal density of }X.$$

The lab uses the Gaussian special case, with $\hat\tau^2=\max(0,\overline{X^2}-1)$ estimated from all $m$ observations. That is honest empirical Bayes, not an oracle.

Where it breaks

Bayesian immunity to selection holds only to the extent that the prior is right, and with small $m$ the prior is poorly estimated. Try $m=2$. Selective intervals can be extremely wide when the observation is near the selection boundary. Sample splitting depends on an arbitrary split. "Data carving" and randomized selection (Tian & Taylor, 2018) recover some of the lost power.

Key references

Robbins (1956); Dawid (1994); Efron, "Tweedie's formula and selection bias," JASA (2011); Berk, Brown, Buja, Zhang & Zhao, Ann. Statist. (2013); Fithian, Sun & Taylor (2014); Lee, Sun, Sun & Taylor, Ann. Statist. (2016); Tibshirani et al. (2016).

Lab · Report the winner, then cover it
Naive $X_{i^*}\pm1.96$ Sample split Empirical Bayes posterior
Each dot is the error (estimate − true θ) for the selected unit in one simulated study. The vertical bar is the mean error, that is, the selection bias. Each split half has noise variance 2, so the split interval is $X^{(2)}_j\pm1.96\sqrt2$.
Part IV

Resampling & smoothing

Two ways to let the data define the model: resample it, or smooth it. Both come with exact conditions for when they work, and with rates that make the cost of flexibility precise.

08

When the bootstrap works, and when it fails

The bootstrap is consistent when the statistic is a smooth (Hadamard-differentiable) functional of $F$. When it isn't, the failure is silent.

Statement

The bootstrap approximates the law of $r_n\{T(F_n)-T(F)\}$ by the conditional law of $r_n\{T(F_n^*)-T(F_n)\}$. If $T$ is Hadamard differentiable at $F$ tangentially to the support of the Donsker limit, then the functional delta method and the bootstrap Donsker theorem (Giné & Zinn, 1990) imply consistency. For asymptotically pivotal statistics (studentized), the bootstrap is second-order correct: the coverage error is $O(n^{-1})$, compared with $O(n^{-1/2})$ for the normal approximation (Hall, 1992). This is the theoretical basis for the bootstrap-$t$ and BCa intervals.

A canonical failure

Take $X_i\sim\mathrm U(0,\theta)$ and $\hat\theta=X_{(n)}$. Then $n(\theta-\hat\theta)/\theta\rightsquigarrow\mathrm{Exp}(1)$, a continuous law. But the resampled maximum equals $\hat\theta$ whenever the largest observation is drawn:

$$P^*\big(\hat\theta^*=\hat\theta\big)=1-(1-1/n)^n\ \longrightarrow\ 1-e^{-1}\approx0.632 .$$

The bootstrap law has an atom at 0 that the true law doesn't, so it is inconsistent. The fix is the $m$-out-of-$n$ bootstrap ($m\to\infty$, $m/n\to0$) or subsampling, which needs only that a limit law exists (Politis & Romano, 1994).

Where it breaks

Extremes; heavy tails with infinite variance, where the bootstrap mean is inconsistent (Athreya, 1987); parameters on the boundary (Andrews, 2000); non-differentiable functionals such as $|\mu|$ at $\mu=0$; and post-selection or shrinkage estimators such as the lasso. Dependence breaks the naive bootstrap, and the remedies are block, wild and sieve bootstraps.

Key references

Efron (1979, 1987); Bickel & Freedman (1981); Singh (1981); Athreya (1987); Giné & Zinn (1990); Hall, The Bootstrap and Edgeworth Expansion (1992); Politis & Romano (1994); Bickel, Götze & van Zwet (1997); Andrews (2000).

Lab · Bootstrapping the sample maximum
Bootstrap $m(\hat\theta-\hat\theta^*)$, continuous part True limit $\mathrm{Exp}(1)$
The coverage run builds the one-sided 95% bound $\hat\theta+\hat q_{0.95}/n$ from each method's bootstrap quantile, with 300 resamples per dataset.
09

Smoothing & minimax rates

Nonparametric estimation trades bias against variance at rates set by smoothness. The curse of dimensionality is a statement about those rates.

Statement

For the kernel density estimator $\hat f_h(x)=\frac1{nh}\sum_iK\big(\frac{x-X_i}h\big)$ with a second-order kernel, the bias is $\tfrac12h^2\mu_2(K)f''(x)+o(h^2)$ and the variance is $R(K)f(x)/(nh)+o((nh)^{-1})$. Integrating,

$$\mathrm{AMISE}(h)=\frac{R(K)}{nh}+\frac{h^4\mu_2(K)^2R(f'')}{4},\qquad h^*\propto n^{-1/5},\qquad \mathrm{MISE}^*\asymp n^{-4/5}.$$

Stone (1980, 1982) showed this is optimal. Over Hölder classes of smoothness $\beta$ in $d$ dimensions, the minimax rate for squared error is $n^{-2\beta/(2\beta+d)}$. Holding $\beta$ fixed, the exponent goes to zero as $d$ grows, and that is the precise content of the "curse of dimensionality." Nonparametric rates are bought with structure: additivity, sparsity, single-index models, or low intrinsic dimension.

Choosing $h$

Least-squares cross-validation minimizes $\int\hat f_h^2-\frac2n\sum_i\hat f_{h,-i}(X_i)$, which is unbiased for $\mathrm{MISE}(h)-\int f^2$. In a single sample it differs from $\mathrm{ISE}(h)-\int f^2$ by a term of order $n^{-1/2}$ that hardly depends on $h$, so its level drifts while its minimizer tracks $h^*$. Even that minimizer is notoriously noisy: $\hat h/h^*-1=O_p(n^{-1/10})$ (Hall & Marron, 1987). Plug-in selectors (Sheather & Jones, 1991) trade some of that variance for bias. Silverman's rule of thumb assumes $f$ is Gaussian and oversmooths multimodal densities, which the lab shows.

Where it breaks

Boundaries (bias of order $h$, not $h^2$), heavy tails, and densities with locally varying smoothness, where a single global $h$ is wrong somewhere. Higher-order kernels reduce bias but can produce negative density estimates. Confidence bands need undersmoothing or explicit bias correction, because at $h^*$ the bias and the standard deviation have the same order (Calonico, Cattaneo & Farrell, 2018).

Key references

Rosenblatt (1956); Parzen (1962); Stone (1980, 1982); Rudemo (1982); Bowman (1984); Hall & Marron (1987); Silverman (1986); Sheather & Jones (1991); Tsybakov, Introduction to Nonparametric Estimation (2009).

Lab · Bandwidth and integrated squared error
True $f$: $0.6\,N(0,1)+0.4\,N(2.2,0.5^2)$ $\hat f_h$
Error criteria vs. bandwidth (log–log)
ISE (oracle) LSCV $+\int f^2$ (data only; its level is noisy, its minimizer is what counts) Silverman's rule
Part V

High dimensions

When $p$ grows with $n$, fixed-dimensional intuition fails. Consistency needs structure such as sparsity, and even the identity covariance looks distorted. Stein's paradox (idea 4) was the first sign of this.

10

The lasso & sparsity

With more variables than observations, sparsity and ℓ₁ convexity make estimation possible, but only under conditions on the design that are easy to violate.

Statement

$\hat\beta_\lambda=\arg\min_\beta\ \frac1{2n}\|y-X\beta\|_2^2+\lambda\|\beta\|_1$. Suppose $\beta$ is $s$-sparse, the noise is Gaussian with variance $\sigma^2$, and $X$ satisfies a restricted eigenvalue condition with constant $\kappa$. Taking $\lambda\asymp\sigma\sqrt{\log p/n}$ gives, with high probability (Bickel, Ritov & Tsybakov, 2009),

$$\|\hat\beta-\beta\|_2^2\ \lesssim\ \frac{\sigma^2}{\kappa^2}\cdot\frac{s\log p}{n}.$$

The $\log p$ factor is the whole price of not knowing the support. Exact support recovery needs more. You need a beta-min condition, and the irrepresentable condition (Zhao & Yu, 2006; Wainwright, 2009):

$$\big\|X_{S^c}^\top X_S\,(X_S^\top X_S)^{-1}\operatorname{sign}(\beta_S)\big\|_\infty\ \lt\ 1 .$$

Why it's true

The choice $\lambda\ge2\|X^\top\varepsilon/n\|_\infty$, which holds with high probability at the $\sqrt{\log p/n}$ scale by a union bound over $p$ Gaussians, forces the error into a cone $\|\Delta_{S^c}\|_1\le3\|\Delta_S\|_1$. On that cone the restricted eigenvalue condition makes the quadratic loss strongly convex. Coordinate descent with soft-thresholding $S_\lambda(z)=\operatorname{sign}(z)(|z|-\lambda)_+$ and warm starts computes the whole path cheaply (Friedman, Hastie & Tibshirani, 2010). The lab uses it.

Where it breaks

Correlated designs violate irrepresentability, and the lasso then selects the wrong variables even with infinite data. Raise $\rho$ and watch. Estimates are biased toward zero, so naive post-lasso inference is invalid. Remedies include debiasing (Zhang & Zhang, 2014; van de Geer et al., 2014; Javanmard & Montanari, 2014), selective inference (idea 7) and stability selection.

Key references

Tibshirani (1996); Donoho & Johnstone (1994); Chen, Donoho & Saunders (1998); Meinshausen & Bühlmann (2006); Zhao & Yu (2006); Candès & Tao (2007); Bickel, Ritov & Tsybakov (2009); Wainwright (2009, 2019); Friedman, Hastie & Tibshirani (2010).

Lab · Lasso path, n = 60, p = 150, s = 6
True nonzero coefficients True zeros Theory $\lambda=\sigma\sqrt{2\log p/n}$
The design is equicorrelated, $X_{ij}=\sqrt\rho\,Z_i+\sqrt{1-\rho}\,E_{ij}$, with columns standardized. The irrepresentable index is the left-hand side of the condition above, computed for this design. Values above 1 mean the lasso can't recover the support exactly at any $\lambda$.
11

Random matrix theory

When the dimension grows with the sample size, the sample covariance is not a noisy version of the truth. Its eigenvalues spread out in a deterministic way.

Statement

Let $X\in\mathbb R^{n\times p}$ have iid $N(0,1)$ entries, so $\Sigma=I_p$, and let $S=X^\top X/n$. If $p/n\to\gamma\in(0,1]$, the empirical spectral distribution of $S$ converges almost surely to the Marchenko–Pastur law:

$$f_\gamma(x)=\frac{\sqrt{(b-x)(x-a)}}{2\pi\gamma x}\,\mathbf 1_{[a,b]}(x),\qquad a=(1-\sqrt\gamma)^2,\quad b=(1+\sqrt\gamma)^2 .$$

Every population eigenvalue equals 1, yet the sample eigenvalues fill $[a,b]$. The largest one converges to $b$ with Tracy–Widom fluctuations of order $n^{-2/3}$ (Johnstone, 2001). Spiked model: a population spike $\ell$ produces an outlier sample eigenvalue only if $\ell\gt1+\sqrt\gamma$, the BBP phase transition. In that case the outlier sits at $\ell(1+\gamma/(\ell-1))$, and the squared cosine between the sample and population eigenvectors converges to $\frac{1-\gamma/(\ell-1)^2}{1+\gamma/(\ell-1)}$.

Why it matters

PCA is inconsistent when $p\asymp n$. Plug-in Markowitz portfolios underestimate risk. Hotelling's $T^2$ loses power and then can't be computed. Covariance shrinkage, either linear (Ledoit & Wolf, 2004) or nonlinear, which inverts the MP map, is the principled response. The proofs use the Stieltjes transform $m(z)=\int\frac{dF(x)}{x-z}$, which satisfies a quadratic self-consistency equation.

Where it breaks

Heavy-tailed entries (fewer than four moments) change the edge behavior. Dependence across rows or a non-identity $\Sigma$ changes the limit to a generalized MP law, which is the setting for nonlinear shrinkage. For $\gamma\gt1$ there are $p-n$ exact zero eigenvalues.

Key references

Wishart (1928); Marchenko & Pastur (1967); Johnstone, Ann. Statist. (2001); Dumitriu & Edelman (2002); Ledoit & Wolf (2004, 2012); Baik, Ben Arous & Péché (2005); Paul (2007); Bai & Silverstein, Spectral Analysis of Large Dimensional Random Matrices (2010).

Lab · Eigenvalues of $S$ when $\Sigma = I$
Eigenvalues of $S$ ($p = 300$) Marchenko–Pastur density True eigenvalue (all = 1)
The eigenvalues are sampled exactly using the Dumitriu–Edelman bidiagonal model: the eigenvalues of $BB^\top/n$, where $B$ has $\chi_{n},\chi_{n-1},\dots$ on the diagonal and $\chi_{p-1},\dots,\chi_1$ below it, have the same law as those of $S$. They are computed by Sturm-sequence bisection, so even $n=15{,}000$ runs instantly.
Part VI

Causal inference

Once identification is settled, causal estimation is a semiparametric problem: a low-dimensional target with infinite-dimensional nuisance functions. Influence functions show how to estimate the target at $\sqrt n$ rates when the nuisances can only be learned slowly.

12

Double robustness & semiparametric efficiency

Estimate a causal effect using two nuisance models and you need only one of them to be right. If both are good, you reach the efficiency bound.

Statement

Observe $O=(X,A,Y)$ and target $\tau=\mathbb E[Y(1)-Y(0)]$. Under consistency, unconfoundedness $Y(a)\perp\!\!\!\perp A\mid X$ and overlap $0\lt e(X)\lt1$, the effect is identified by both $\mathbb E[\mu_1(X)-\mu_0(X)]$ and $\mathbb E\big[\frac{AY}{e(X)}-\frac{(1-A)Y}{1-e(X)}\big]$. The efficient influence function (Hahn, 1998) is

$$\begin{aligned}\varphi(O)=\ &\mu_1(X)-\mu_0(X)-\tau\\ &+\frac{A\{Y-\mu_1(X)\}}{e(X)}-\frac{(1-A)\{Y-\mu_0(X)\}}{1-e(X)},\end{aligned}$$

and AIPW is the plug-in sample mean of $\varphi+\tau$. Its bias is a product of nuisance errors:

$$\hat\tau_{\mathrm{AIPW}}-\tau\ \approx\ (\mathbb P_n-P)\varphi\ +\ O_p\!\Big(\|\hat e-e\|_{2}\,\big\|\hat\mu-\mu\big\|_{2}\Big).$$

Why it matters

If either $\hat e$ or $\hat\mu$ is consistent, the product goes to zero, which is model double robustness. If both converge faster than $n^{-1/4}$, the product is $o_p(n^{-1/2})$, and AIPW attains the semiparametric efficiency bound $\operatorname{Var}\varphi$ even when the nuisances come from flexible machine-learning fits. That is rate double robustness, and it is the foundation of double/debiased ML. Cross-fitting removes the Donsker condition on the nuisance estimators (Chernozhukov et al., 2018). The same "Neyman orthogonality" principle drives TMLE.

Where it breaks

If both models are wrong, AIPW is biased, and with near-violations of overlap its inverse weights make it more variable than plain regression (Kang & Schafer, 2007). Trimming and overlap weights trade bias for variance. And no estimator can fix unmeasured confounding: double robustness concerns the estimation step, not the identification assumptions.

Key references

Rosenbaum & Rubin (1983); Robins, Rotnitzky & Zhao, JASA (1994); Hahn (1998); Scharfstein, Rotnitzky & Robins (1999); Bang & Robins (2005); van der Laan & Rubin (2006), TMLE; Kang & Schafer (2007); Tsiatis, Semiparametric Theory and Missing Data (2006); Chernozhukov et al., Econometrics J. (2018).

Lab · Misspecify the nuisances

The truth: $\mathrm{logit}\,e(X)=0.6X_1+0.6(X_2^2-1)$ and $Y=2+\tau A+X_1+1.5(X_2^2-1)+\varepsilon$, with $\tau=1$. A "misspecified" model is linear in $(X_1,X_2)$ and omits $X_2^2$. Each study has $n=1{,}000$.

Outcome model
Propensity model
Try all four combinations. AIPW stays centered unless both models are wrong. IPW uses the normalized (Hájek) form, and propensities are clipped to $[0.01, 0.99]$.
Synthesis

Four threads through the twelve

Local quadratic approximation

LAN underlies Fisher efficiency, Wilks, the delta method and bootstrap consistency (ideas 1, 2, 8). Every failure here is a failure of the quadratic: boundaries, discreteness, non-smooth functionals.

Pointwise vs. uniform

Superefficiency, post-selection inference, FDR and empirical processes (ideas 1, 3, 6, 7) all turn on the difference between holding for each $\theta$ and holding uniformly over $\theta$, or over hypotheses, or over function classes.

The price of dimension

Stein shrinkage, Stone's rates, $s\log p/n$ and Marchenko–Pastur (ideas 4, 9–11) each put a number on how fixed-$p$ intuition fails, and each points to structure (sparsity, smoothness, exchangeability) as the way out.

Influence functions & orthogonality

Efficient scores, AIPW and debiased ML (ideas 1, 10, 12) build estimators whose first-order error doesn't depend on the nuisances. That is how slowly learned nuisances can still give $\sqrt n$ inference.

A reading list

  • A. W. van der Vaart, Asymptotic Statistics (1998). LAN, efficiency, the delta method, empirical processes and the bootstrap in one rigorous volume.
  • E. L. Lehmann & G. Casella, Theory of Point Estimation (2nd ed., 1998), and Lehmann & Romano, Testing Statistical Hypotheses (4th ed., 2022).
  • A. W. van der Vaart & J. A. Wellner, Weak Convergence and Empirical Processes (1996; 2nd ed., 2023).
  • M. J. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint (2019). Concentration, the lasso and random matrices.
  • B. Efron, Large-Scale Inference (2010). Empirical Bayes, FDR and Tweedie's formula.
  • A. B. Tsybakov, Introduction to Nonparametric Estimation (2009). Minimax lower bounds done properly.
  • C. P. Robert & G. Casella, Monte Carlo Statistical Methods (2nd ed., 2004).
  • A. A. Tsiatis, Semiparametric Theory and Missing Data (2006), and M. A. Hernán & J. M. Robins, Causal Inference: What If (2020).