Why a Different Scale Is Needed
For a smooth scalar functional \(g(\theta)\), the ordinary delta method uses the linear change in \(g\) near the true parameter \(\theta_0\). If the gradient vanishes at \(\theta_0\), that linear change is zero. A first-order approximation then does not describe the leading random variation: curvature, rather than slope, becomes decisive. The functional often fluctuates on the scale \(n^{-1}\), not \(n^{-1/2}\).
This situation occurs naturally when estimating a squared distance from a hypothesized value, a variance-like functional at a symmetry point, or a contrast whose first derivative vanishes at the parameter of interest. The second-order delta method identifies both the appropriate scale and the shape of the limiting distribution.
Suppose an estimator \(\hat{\theta}\) is consistent and satisfies \(\sqrt n(\hat{\theta}-\theta_0)\xrightarrow{d}Z\), where \(Z\sim N_p(0,V)\) and \(V\) is a finite, symmetric positive semidefinite matrix. At a stationary point, the first-order term disappears. The next result makes precise what replaces it.
The Second-Order Delta Method
The estimator’s root-\(n\) limit is still the input to the calculation. The output scale changes because the functional’s first derivative is zero: a quadratic change in an \(O_p(n^{-1/2})\) estimation error is \(O_p(n^{-1})\).
Why the Limit Is a Weighted Chi-Square
The quadratic form in the theorem can be expressed using the eigenvalues of a matrix built from the Hessian and the asymptotic covariance. This representation identifies whether the limit is a nonnegative weighted chi-square or a signed combination of chi-squares.
The covariance matters as much as the curvature. Directions in which the estimator has little or no asymptotic variation contribute little or nothing to the limit, even if the functional curves in those directions. The eigenvalues combine both effects, so inspecting the Hessian alone is not enough to determine the limiting weights.
Worked Example: Squared Error at a Bernoulli Symmetry Point
Let \(X_1,\ldots,X_n\) be independent Bernoulli observations with success probability \(p\), and estimate \(p\) by \(\hat p=\bar X\). Consider \(g(p)=(p-\tfrac12)^2\) when the true value is \(p_0=\tfrac12\).
The derivative is \(g'(p)=2(p-\tfrac12)\), so \(g'(p_0)=0\); the second derivative is \(g''(p)=2\). The central limit theorem gives \(\sqrt n(\hat p-\tfrac12)\xrightarrow{d}Z\), where \(Z\sim N(0,\tfrac14)\), because \(p_0(1-p_0)=\tfrac14\). The second-order limit is therefore $$ n\{g(\hat p)-g(p_0)\} =n(\hat p-\tfrac12)^2 \xrightarrow{d} Z^2 \overset{d}{=}\frac14\chi^2_1. $$ The factor \(\tfrac14\) follows by writing \(Z=\tfrac12 W\) for \(W\sim N(0,1)\). Here \(g(p_0)=0\), so the result describes the scaled squared estimation error itself.
Worked Example: Two Curvature Directions with Different Variances
Suppose \(Y_1,\ldots,Y_n\) are independent bivariate normal vectors with mean \(\theta_0=(0,0)^{\mathsf T}\) and covariance \(V=\operatorname{diag}(1,4)\). Use their sample mean \(\hat{\theta}\) to estimate \(\theta_0\), and consider \(g(\theta)=\theta_1^2+\tfrac12\theta_2^2\).
The sample mean satisfies \(\sqrt n\,\hat{\theta}\sim N_2(0,V)\) exactly. The gradient of \(g\) vanishes at \(\theta_0\), and its Hessian is \(H=\operatorname{diag}(2,1)\). If \(Z=(Z_1,Z_2)^{\mathsf T}\sim N_2(0,V)\), then \(Z_1=W_1\) and \(Z_2=2W_2\) for independent standard normal variables \(W_1,W_2\). Direct substitution gives $$ n\{g(\hat{\theta})-g(\theta_0)\} \xrightarrow{d} \frac12 Z^{\mathsf T}HZ =Z_1^2+\frac12 Z_2^2 \overset{d}{=}W_1^2+2W_2^2. $$ The eigenvalues of \(V^{1/2}HV^{1/2}=\operatorname{diag}(2,4)\) are \(2\) and \(4\), producing weights \(1\) and \(2\) after multiplication by \(\tfrac12\). Unequal variances in the two coordinates lead to unequal limiting weights.
Worked Example: A Stationary Point with Opposite Curvatures
Let \(Y_1,\ldots,Y_n\) be independent bivariate normal vectors with mean \((0,0)^{\mathsf T}\) and covariance \(I_2\). Take \(\hat{\theta}=\bar Y\) and \(g(\theta)=\theta_1^2-\theta_2^2\). The gradient vanishes at \(\theta_0=(0,0)^{\mathsf T}\), and \(H=\operatorname{diag}(2,-2)\).
Here \(V=I_2\), so the eigenvalues of \(V^{1/2}HV^{1/2}\) are \(2\) and \(-2\). For independent \(W_1,W_2\sim N(0,1)\), the limit is $$ n\{g(\hat{\theta})-g(\theta_0)\} \xrightarrow{d} W_1^2-W_2^2 \overset{d}{=}\chi^2_{1,1}-\chi^2_{1,2}, $$ where the two chi-square variables are independent. The limiting variable can be positive or negative because the functional curves upward in one direction and downward in the other. Calling this limit a chi-square distribution would be incorrect.
Beyond Second Order
If the Hessian contributes no variation, the second-order limit may be identically zero. For example, this happens if \(V^{1/2}HV^{1/2}=0\), even when \(H\) itself is not zero. In that case the second-order theorem is valid but does not identify a nondegenerate limit; a higher-order expansion may be needed.
More generally, suppose \(g\) has continuous derivatives through order \(r\) near \(\theta_0\), its derivatives of orders \(1,\ldots,r-1\) vanish there, and \(\sqrt n(\hat{\theta}-\theta_0)\xrightarrow{d}Z\). Taylor expansion then yields $$ n^{r/2}\{g(\hat{\theta})-g(\theta_0)\} \xrightarrow{d} \frac{1}{r!}D^rg(\theta_0)[Z,\ldots,Z], $$ where \(D^rg(\theta_0)[Z,\ldots,Z]\) is the \(r\)-th derivative, viewed as a multilinear form, evaluated \(r\) times at \(Z\). As in the second-order proof, the Taylor remainder is \(o_p(\lVert\hat{\theta}-\theta_0\rVert^r)\), and root-\(n\) tightness makes its product with \(n^{r/2}\) vanish in probability. For \(r=2\), this expression is precisely the Hessian quadratic form.
Common Mistakes and Practical Interpretation
A frequent error is to apply the ordinary delta method mechanically and conclude that a zero gradient means there is no asymptotic variation. It means only that the \(n^{-1/2}\)-scale linear term vanishes. The next term can still be random, and the correct scale for the functional may be \(n\).
A second mistake is to assume every quadratic-form limit is chi-square. A chi-square variable is nonnegative, whereas an indefinite Hessian can produce negative eigenvalues and a signed limit. Even when all weights are nonnegative, unequal weights generally give a weighted chi-square, not a single ordinary chi-square. The eigenvalues of \(V^{1/2}HV^{1/2}\), including their signs and zeros, are the relevant diagnostic.
These limits matter for inference because they describe the sampling behavior of functionals for which a first-order normal approximation fails. They also warn against applying a usual normal confidence interval on the wrong scale. Before using the approximation, check stationarity, the estimator’s joint asymptotic covariance, and the curvature in directions where the estimator varies. If the quadratic form vanishes, the result gives no nondegenerate approximation by itself.
Check Your Understanding
Use the conditions and calculations in the tutorial to answer the following.
- Why does a zero gradient at \(\theta_0\) change the natural scaling of \(g(\hat{\theta})-g(\theta_0)\) from \(n^{1/2}\) to \(n\)?
- For the second-order limit, which matrix’s eigenvalues determine the chi-square weights, and why does the asymptotic covariance appear in that matrix?
- What property of the eigenvalues ensures that the limiting quadratic form is nonnegative?
- Can a nonzero Hessian still yield a degenerate second-order limit? State the relevant condition involving \(V\) and \(H\).
- If the first nonzero derivative of \(g\) at \(\theta_0\) has order \(r\), what is the corresponding scale for the functional difference under a root-\(n\) estimator?