From Information to Parameter Uncertainty
An information matrix is useful not only for comparing designs but also for anticipating how precisely parameters can be estimated. A design with substantial information in every relevant parameter direction tends to produce smaller estimator variances. The inverse Fisher information gives a local, large-sample approximation to the covariance matrix of a maximum likelihood estimator (MLE). Its diagonal entries yield approximate variances; their square roots are asymptotic standard errors.
This connection is an approximation, not a promise that an estimator has an exactly normal distribution or that its finite-sample variance equals the inverse information. Its usefulness depends on regularity conditions and on the model and parameter values used to calculate the information. In nonlinear pharmacometric models, the approximation is often local: it describes uncertainty near a specified parameter value or fitted estimate.
Here \(I(\theta)\) denotes the information for all observations in the analysis. If independent observations contribute information additively, total information is the sum of their contributions. With \(n\) identically distributed independent observations, it is often \(n\) times the per-observation information. For an approximate design with per-subject information \(I(\xi;\theta)\), \(n\) subjects give total information \(nI(\xi;\theta)\), and the approximate covariance is \([nI(\xi;\theta)]^{-1}\). Be clear about whether a reported matrix is per subject or already total; otherwise the factor of \(n\) can be omitted or counted twice.
Why the Inverse Appears
The inverse-information result follows from a first-order approximation to the score equation. Suppose the true parameter \(\theta_0\) is an interior point, the model is correctly specified and identifiable, the likelihood is sufficiently smooth, and the observations provide increasing information. The MLE approximately solves \(U(\hat{\theta})=0\). A Taylor expansion around \(\theta_0\) gives
The derivative of the score is the Hessian of the log-likelihood. For a large sample it is approximately \(-I(\theta_0)\), while the score has mean zero and covariance \(I(\theta_0)\). Rearranging the expansion therefore gives
This justification also shows why the approximation is sensitive to assumptions: it relies on a well-behaved score, a locally quadratic log-likelihood, and an invertible information matrix. In applications, the unknown \(\theta_0\) is usually replaced by \(\hat{\theta}\), giving the estimated covariance approximation \(I(\hat{\theta})^{-1}\). With a design calculation, the matrix may instead be evaluated at a nominal parameter vector. The result is then a prediction of precision conditional on that model and parameter vector.
Standard Errors and Wald Confidence Intervals
For a \(p\)-dimensional parameter vector, let \(\widehat V=I(\hat{\theta})^{-1}\) be the estimated covariance approximation. The standard error for component \(\hat{\theta}_j\) is the square root of the \(j\)th diagonal element of \(\widehat V\). Off-diagonal elements describe approximate covariances, so parameter estimates can be strongly correlated even when each has a finite standard error. A diagonal entry of the information matrix itself is not, in general, the variance or the reciprocal variance for that component: the full matrix must be inverted when parameters are correlated.
For a scalar parameter, or one component of a parameter vector, an approximate two-sided \(100(1-\alpha)\%\) Wald confidence interval is
where \(z_{1-\alpha/2}\) is the corresponding standard normal quantile. For a 95% interval, \(z_{0.975}\) is approximately 1.96. The interval is justified by the approximate normal sampling distribution of the estimator, not by a claim that the fixed parameter has a 95% probability of lying in this particular interval. In repeated comparable analyses, the procedure has approximately 95% coverage when its assumptions and approximation are adequate.
Worked Example: Standard Error for a Normal Mean
Suppose, hypothetically, that \(n=25\) independent measurements follow \(X_i\sim N(\mu, 2^2)\), with the measurement standard deviation known to be 2 units. The observed sample mean is \(\bar{x}=10.8\) units. Under this model, the likelihood information for \(\mu\) is \(n/\sigma^2\). The normal model, independence, and known variance are stipulated here, so this calculation is conditional on those assumptions.
Thus \(SE(\bar{x})=\sqrt{0.1600}=0.4000\) units. The 95% Wald interval is
Under repeated sampling from the stated normal model, this procedure has 95% coverage; for known variance and normal observations, the interval is also an exact normal-theory interval. This special exactness should not be assumed for general nonlinear likelihoods, where inverse information and Wald coverage are usually asymptotic.
Reading a Multivariate Covariance Approximation
For a vector parameter, uncertainty in one component must be calculated after accounting for the other estimated parameters. The following hypothetical information matrix is a total information matrix for two parameters: \(\theta_1\), a clearance in L/h, and \(\theta_2\), a volume in L. Suppose the fitted values are \(2.00\) L/h and \(0.500\) L. Assume the likelihood is regular and locally well approximated by a quadratic around these interior estimates; the example illustrates the resulting Wald calculation, not evidence that the assumptions hold in a particular study.
Worked Example: Inverting a Two-Parameter Information Matrix
The information matrix and its determinant are
Since the determinant is positive and the first diagonal entry is positive, this symmetric \(2\times2\) matrix is positive definite and invertible. Its inverse is
The approximate standard errors are the square roots of the diagonal entries: \(SE(\hat{\theta}_1)=\sqrt{0.03906}=0.1976\) L/h and \(SE(\hat{\theta}_2)=\sqrt{0.1563}=0.3953\) L. The corresponding componentwise 95% Wald intervals are
The negative lower endpoint for a volume is not a physically plausible value. It signals that the symmetric normal approximation is broad relative to the positive parameter space; it does not mean a negative volume is physically possible. The off-diagonal covariance also matters: the approximate correlation is \(-0.04688/\sqrt{(0.03906)(0.1563)}=-0.600\). Thus, the two estimates are negatively correlated in this local approximation. Reporting only their standard errors would omit this feature of joint uncertainty.
For a linear contrast \(c^T\theta\), where \(c\) is a fixed vector, the approximate variance is \(c^T\widehat Vc\), and its standard error is the square root of that quantity. This is useful when the target is a combination of parameters rather than a single component. For a nonlinear transformation \(g(\theta)\), a first-order Taylor expansion gives the delta-method variance approximation
Alternatively, for a strictly increasing transformation of a scalar parameter, one can transform both endpoints of a confidence interval on the original parameter scale. The resulting interval need not be symmetric around the transformed estimate.
Worked Example: A Confidence Interval on the Exponentiated Scale
Suppose a hypothetical positive parameter is represented as \(\theta=\exp(\beta)\) L/h, and the fitted log-scale parameter is \(\hat{\beta}=1.3863\) with \(SE(\hat{\beta})=0.2000\). Then \(\hat{\theta}=\exp(1.3863)\approx4.000\) L/h. Assume the log-scale likelihood estimate is sufficiently close to normal for a Wald interval to be informative.
First calculate the 95% interval for \(\beta\):
Because exponentiation is increasing, exponentiating the endpoints gives an interval for \(\theta\):
This interval is asymmetric around \(4.000\) L/h, which is expected after exponentiation. Its approximate coverage depends on the log-scale normal approximation. It is not obtained by adding and subtracting \(1.96\) times a standard error on the original scale.
Assumptions, Diagnostics, and Alternatives
The inverse-information approximation is most defensible when the model is correctly specified, parameters are identifiable and away from problematic boundaries, the likelihood is smooth, and the data provide enough information for a local quadratic approximation. In a design calculation, these claims are conditional on the assumed observation model and nominal parameter values. A large number of observations alone does not resolve nonidentifiability or misspecification.
Inspect the fitted model and uncertainty summaries for warning signs. A singular or nearly singular information matrix, extremely large standard errors, or very strong parameter correlations may indicate that some parameter combinations are weakly informed. A Wald interval that extends far into implausible values, as in the volume example, suggests the symmetric approximation may be misleading. A strongly skewed likelihood, estimates near a boundary, or marked changes in standard errors across plausible parameter values also call for caution. These checks diagnose possible problems; none by itself proves that the model is invalid.
Expected Fisher information averages curvature over possible data under the model. Observed information, the negative Hessian of the log-likelihood at the actual data and fitted estimate, uses the curvature actually observed. Both can be used to form a local covariance approximation, but they can differ in finite samples. The choice should be stated, especially when reporting a matrix calculated by software or a design program.
Wald intervals are computationally simple and directly connected to the inverse information. Profile-likelihood intervals instead examine the likelihood over values of a target parameter while re-optimizing nuisance parameters; they can reflect asymmetry better, though they still depend on a suitable likelihood and can require more computation. A parametric bootstrap simulates data under a fitted model and refits it to approximate an estimator's sampling distribution; it can expose skewness or finite-sample behavior, but inherits the assumed model and may be unstable when refits fail. Robust sandwich covariance estimates can address certain forms of likelihood misspecification in large samples, but do not repair a poor mean model or eliminate weak identification. These alternatives are not automatic fixes; their assumptions and target of inference should be matched to the problem.
Information criteria such as A-, D-, and c-optimality summarize different aspects of the same information matrix, as covered in the earlier material on those criteria. Inference adds an important practical step: translate the matrix into standard errors, covariances, and intervals for specific targets, then judge whether the approximation is plausible on the parameter scale that matters. A design that is optimal under a criterion still relies on the model, parameter values, and asymptotic approximation used to calculate its information.
Check Your Understanding
Try each question, then compare your reasoning with the solutions.
- If an analysis reports total information \(I\) for \(n\) independent subjects, should you multiply \(I^{-1}\) by \(n\) again to obtain the covariance approximation? Explain.
- For an estimated covariance matrix with diagonal entries \(0.09\) and \(0.25\), what are the approximate standard errors of the two parameters?
- Why can a Wald interval for a positive parameter include negative values, and what does that indicate?
- If two parameter estimates have a nonzero covariance, how should the approximate variance of their sum be calculated?
Solutions. (1) No. If \(I\) is already total information, the covariance approximation is \(I^{-1}\); multiplying by \(n\) would incorrectly inflate it. (2) The standard errors are \(\sqrt{0.09}=0.300\) and \(\sqrt{0.25}=0.500\), in the respective parameter units. (3) A Wald interval is symmetric on the estimation scale and can extend beyond the parameter space; this warns that the normal approximation may be poor or imprecise on that scale, rather than implying negative values are physically possible. (4) If the parameters are \(\theta_1,\theta_2\), then \(\operatorname{Var}(\hat{\theta}_1+\hat{\theta}_2)\approx \widehat V_{11}+\widehat V_{22}+2\widehat V_{12}\). The covariance term cannot be omitted unless it is zero.