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 $C$.
Fisher information & the trinity
Efficiency bounds, and why the Wald interval for a proportion is badly behaved.
Wilks' theorem at the boundary
The χ² limit, and the cone geometry that replaces it at the boundary.
Empirical processes
Glivenko–Cantelli, Donsker and DKW: uniform laws for $\mathbb P_n$.
Stein's paradox
In three or more dimensions the MLE is inadmissible, and empirical Bayes explains why.
MCMC & optimal scaling
Detailed balance, ESS and the 0.234 rule.
False discovery rate
Benjamini–Hochberg and the two-groups model.
Inference after selection
The winner's curse, sample splitting, and why Bayes ignores selection.
When the bootstrap fails
Hadamard differentiability, and what goes wrong at the sample maximum.
Smoothing & minimax rates
The $n^{-4/5}$ rate, cross-validation, and the curse of dimensionality.
The lasso & sparsity
$s\log p/n$ rates, and the irrepresentable condition.
Random matrix theory
Marchenko–Pastur: sample eigenvalues spread out even when the truth is the identity.
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.
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:
The modern form of "efficiency" doesn't need unbiasedness. Le Cam's local asymptotic normality (LAN) says that
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 $\hat p$:
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).
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
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
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."
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:
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).
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.
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
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).
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
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).
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.
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
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).
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:
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).
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.
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:
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).
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,
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).
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.
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),
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):
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).
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:
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).
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.
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
and AIPW is the plug-in sample mean of $\varphi+\tau$. Its bias is a product of nuisance errors:
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).
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 $n=1{,}000$.
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).