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Exponential Families and Asymptotics · Tutorial 84 of 975

Wald, Score, and Likelihood-Ratio Equivalence

Learn how the three classical likelihood tests arise from the same local quadratic approximation, and how to calculate and compare them in finite samples.

Intermediate 12 min read

What You'll Learn

  • State regularity conditions for comparing Wald, score, and likelihood-ratio tests.
  • Derive the common chi-square limit for a hypothesis imposing q smooth restrictions.
  • Use efficient information to account for nuisance parameters in the score and Wald statistics.
  • Calculate all three statistics in normal and binomial examples.
  • Identify why asymptotic equivalence does not imply identical finite-sample results.

Three Routes to Testing the Same Hypothesis

For a regular nested hypothesis, three familiar tests ask how strongly the data disagree with the null in different ways. The Wald test measures how far the unrestricted estimate lies from the null. The score test measures the likelihood’s slope at the restricted estimate. The likelihood-ratio test compares the best likelihood available under the null with the unrestricted maximum. Their calculations can look different, but locally they are driven by the same quadratic shape of the log-likelihood.

The equivalence is asymptotic, not an assertion that the statistics are equal for a particular sample. We derive their common limit and then calculate examples where the finite-sample values either coincide or differ. The distinction matters in applications: using a chi-square reference distribution does not erase the effects of sample size, skewness, or nuisance-parameter estimation.

Setup and Regularity Conditions

Let \(X_1,\ldots,X_n\) be independent observations from a correctly specified regular parametric model with log-likelihood \(\ell_n(\theta)\), where \(\theta=(\psi^T,\eta^T)^T\). The parameter of interest \(\psi\) has dimension \(q\), and \(\eta\) is a nuisance parameter. We test the nested hypotheses \(H_0:\psi=\psi_0\) against the unrestricted alternative. The true parameter under the null is \((\psi_0,\eta_0)\).

Regularity conditions: The true parameter is an interior point of an identifiable parameter space; the model is differentiable in quadratic mean with finite, nonsingular Fisher information; the relevant likelihood derivatives obey a uniform local quadratic expansion; and the unrestricted and restricted maximum-likelihood estimators are consistent and root-\(n\) regular. These conditions ensure that the information and score approximations below hold and that the maxima are attained locally. The \(q\) restrictions are independent, so the null has codimension \(q\).

Write the per-observation Fisher information at the null in blocks:

$$ I= \begin{pmatrix} I_{\psi\psi} & I_{\psi\eta}\\ I_{\eta\psi} & I_{\eta\eta} \end{pmatrix}. $$

Assume \(I_{\eta\eta}\) is nonsingular. The efficient information for \(\psi\), after accounting for the nuisance parameter, is the Schur complement \(J=I_{\psi\psi}-I_{\psi\eta}I_{\eta\eta}^{-1}I_{\eta\psi}\), which is positive definite under the stated conditions. This is per-observation information; the corresponding information in \(n\) observations is \(nJ\).

Definition: Let \(\hat\theta=(\hat\psi^T,\hat\eta^T)^T\) be the unrestricted maximum-likelihood estimator, and let \(\tilde\eta\) maximize the likelihood subject to \(\psi=\psi_0\). With \(\hat J_n\) a consistent estimate of the per-observation efficient information \(J\), define

Wald: \(W_n=n(\hat\psi-\psi_0)^T\hat J_n(\hat\psi-\psi_0)\).
Score: \(S_n=U_\psi^T(n\hat J_n)^{-1}U_\psi\), where \(U_\psi=\partial\ell_n(\psi_0,\tilde\eta)/\partial\psi\).
Likelihood ratio: \(R_n=2\{\ell_n(\hat\theta)-\ell_n(\psi_0,\tilde\eta)\}\).

At the restricted maximum, the nuisance score is zero. The score statistic therefore uses the score in the tested directions and the total efficient information \(n\hat J_n\), not just per-observation information. Equivalently, \(S_n=(U_\psi/\sqrt n)^T\hat J_n^{-1}(U_\psi/\sqrt n)\).

Why the Statistics Have the Same Limit

The key is the local likelihood after nuisance parameters have been adjusted to their best-fitting values. For bounded \(h\), consider changing \(\psi\) from \(\psi_0\) to \(\psi_0+h/\sqrt n\), while maximizing over the nuisance parameter. The regular likelihood expansion gives

$$ \ell_{p,n}(\psi_0+h/\sqrt n)-\ell_{p,n}(\psi_0) = h^T\Delta_n-\frac12h^TJh+o_p(1), $$

uniformly over bounded \(h\). Here \(\ell_{p,n}\) denotes the likelihood with the nuisance parameter locally optimized, and \(\Delta_n=U_\psi/\sqrt n\) at the restricted fit. Under the null, \(\Delta_n\xrightarrow{d}N(0,J)\). In particular, the nuisance adjustment is essential: the covariance of this adjusted score is \(J\), not generally \(I_{\psi\psi}\).

Theorem: Under the regularity conditions above, under \(H_0\), \(W_n\), \(S_n\), and \(R_n\) each converge in distribution to a chi-square random variable with \(q\) degrees of freedom. More precisely, their pairwise differences converge to zero in probability.

Derivation. The quadratic expression in the local expansion is maximized at \(h=J^{-1}\Delta_n\). Its maximum is \(\frac12\Delta_n^TJ^{-1}\Delta_n\). The unrestricted estimate has local displacement \(\sqrt n(\hat\psi-\psi_0)=J^{-1}\Delta_n+o_p(1)\), as follows from the local score equation. Thus the likelihood-ratio statistic is

$$ R_n=\Delta_n^TJ^{-1}\Delta_n+o_p(1). $$

For the score statistic, \(U_\psi/\sqrt n=\Delta_n\), and consistency gives \(\hat J_n\xrightarrow{p}J\). Hence \(S_n=\Delta_n^TJ^{-1}\Delta_n+o_p(1)\). For the Wald statistic, substitute the local displacement of the unrestricted estimate and the same consistent information estimate:

$$ W_n=(J^{-1}\Delta_n)^TJ(J^{-1}\Delta_n)+o_p(1) =\Delta_n^TJ^{-1}\Delta_n+o_p(1). $$

Finally, write \(Z_n=J^{-1/2}\Delta_n\). Since \(\Delta_n\xrightarrow{d}N(0,J)\), \(Z_n\xrightarrow{d}N(0,I_q)\), and \(\Delta_n^TJ^{-1}\Delta_n=Z_n^TZ_n\xrightarrow{d}\chi_q^2\). Slutsky’s theorem completes the argument for all three statistics. \(\square\)

This derivation also shows what “equivalence” means: each statistic has the same leading random term under the null, so their differences are \(o_p(1)\). It does not say they have the same value at finite \(n\). Under local alternatives \(\psi=\psi_0+a/\sqrt n\), the same quadratic argument gives a noncentral chi-square limit with noncentrality parameter \(a^TJa\); under the null, \(a=0\), yielding the central chi-square result.

Worked Comparisons

Worked Example: A Normal Mean With Known Variance

Suppose \(X_i\sim N(\mu,4)\), independently, and test \(H_0:\mu=0\). For \(n=25\), suppose the observed sample mean is \(\bar X=0.4\). The unrestricted estimate is \(\hat\mu=0.4\), and the per-observation information for \(\mu\) is \(J=1/4\).

Wald. The statistic is \(n\hat\mu^2J=25(0.4)^2/4=1\).

Score. At the null, \(U_\mu=n\bar X/4=25(0.4)/4=2.5\), and total information is \(nJ=25/4=6.25\). Thus \(S_n=2.5^2/6.25=1\).

Likelihood ratio. The log-likelihood difference between \(\hat\mu=\bar X\) and \(\mu=0\) is \(n\bar X^2/(2\cdot4)\). Therefore \(R_n=2[n(0.4)^2/8]=1\). In this normal model, all three statistics coincide exactly for this sample (and, in fact, for every sample). Their shared chi-square limit is not what makes them equal here; the quadratic log-likelihood does.

Worked Example: A Binomial Probability

Let \(X\sim\operatorname{Binomial}(10,p)\), and test \(H_0:p=0.5\). Suppose \(x=8\), so \(\hat p=8/10=0.8\). The per-observation information is \(J(p)=1/[p(1-p)]\).

Wald. Using the information at the unrestricted estimate, \(\hat J_n=1/[0.8(0.2)]=6.25\). Hence \(W_n=10(0.8-0.5)^2(6.25)=5.625\).

Score. The score at \(p=0.5\) is \(U_p=x/p-(10-x)/(1-p)=8/0.5-2/0.5=12\). The per-observation null information is \(J(0.5)=4\), so the total information is \(10(4)=40\). Thus \(S_n=12^2/40=3.6\).

Likelihood ratio. The binomial coefficient cancels in the likelihood ratio, giving \(R_n=2\{8\log(0.8/0.5)+2\log(0.2/0.5)\}\). The expression is \(2\{8\log(1.6)+2\log(0.4)\}\approx3.854896\), or \(3.855\) to three decimal places.

The three values, \(5.625\), \(3.6\), and \(3.855\), are not equal. For a one-degree-of-freedom chi-square reference, the approximate 5% cutoff is \(3.841\): the Wald and likelihood-ratio values exceed it, while the score value does not. This is a finite-sample illustration, not a contradiction of their common asymptotic null distribution.

Worked Example: A Normal Mean With Unknown Variance

Suppose \(X_i\sim N(\mu,\sigma^2)\) with both parameters unknown, and test \(H_0:\mu=0\). Take \(n=4\) observations \(0,0,0,4\). Then \(\bar X=1\), and the unrestricted maximum-likelihood variance is \(\hat\sigma^2=\frac14\sum_i(X_i-\bar X)^2=(1+1+1+9)/4=3\).

Wald. The per-observation efficient information for \(\mu\) is \(1/\sigma^2\). Using the unrestricted estimate gives \(W_n=n\bar X^2/\hat\sigma^2=4(1)^2/3=4/3\).

Score. Under the restriction \(\mu=0\), the nuisance variance estimate is \(\tilde\sigma^2=\frac14\sum_iX_i^2=16/4=4\). The restricted mean score is \(U_\mu=\sum_iX_i/\tilde\sigma^2=4/4=1\), while the total efficient information is \(n/\tilde\sigma^2=4/4=1\). Thus \(S_n=1^2/1=1\).

Likelihood ratio. The maximized normal log-likelihood is \(-\frac n2\{\log(2\pi\hat\sigma^2)+1\}\); under the restriction, replace \(\hat\sigma^2=3\) with \(\tilde\sigma^2=4\). Therefore \(R_n=n\log(4/3)=4\log(4/3)\approx1.151\). The nuisance estimate changes between the restricted and unrestricted fits, and the three finite-sample statistics differ.

Interpretation and a Common Pitfall

The tests have different practical constructions. Wald is convenient when the unrestricted estimate and its covariance are readily available. The score test needs a fit under the null, but not an unrestricted fit. The likelihood-ratio test requires both fits and compares their likelihoods. Under the regular null and large samples, all use the same local information about the \(q\) tested directions, so the degrees of freedom are \(q\).

Common mistake: mixing total and per-observation information. If \(U_\psi\) is the score from all \(n\) observations, dividing its squared size by per-observation information alone makes the score statistic too large by a factor of \(n\). In the binomial example, \(U_p=12\) and per-observation information is \(4\), but the denominator must be total information \(10(4)=40\), giving \(144/40=3.6\). The incorrect calculation \(144/4=36\) does not have the stated chi-square limit. Equivalently, divide the total score by \(\sqrt n\) and use per-observation information.

The regularity conditions are substantive. A parameter on the boundary, a singular information matrix, or a non-identifiable model can invalidate the ordinary chi-square conclusion. In regular problems, finite-sample discrepancies remain possible; the approximation improves asymptotically, but it is not an algebraic identity among the tests.

Check Your Understanding

Use the definitions and derivation above to answer these questions.

  1. Why does the score statistic use total information \(n\hat J_n\) when its numerator is the score from all \(n\) observations?
  2. What role does the efficient information \(J\) play when nuisance parameters are present?
  3. For \(q\) independent smooth restrictions, what is the null limiting distribution of each of the three statistics?
  4. In the binomial example, verify the score statistic using the standardized score \(U_p/\sqrt n\) and per-observation information.
  5. Why do the three statistics coincide in the known-variance normal example but differ in the binomial example?
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