Fisher Information and the Score

How much can a single observation tell us about an unknown parameter? A measurement from a sharply peaked distribution pins down its parameter tightly. A measurement from a diffuse, flat distribution reveals almost nothing. Fisher information makes this vague idea precise. It turns "how informative is my data" into a single computable number attached to a statistical model. It is the quantitative backbone of Maximum Likelihood Estimation. It measures the curvature of the log-likelihood. It predicts the variance of the maximum likelihood estimator. It also sets the ultimate speed limit on how well any estimator can perform. The central actor is the score function — the derivative of the log-likelihood with respect to the parameter. The score is zero on average at the true parameter value. The spread of the score around zero is exactly the Fisher information. This single quantity threads together three seemingly different ideas. These are the sensitivity of the likelihood to the parameter, the variance of an optimal estimator, and the geometry of the family of distributions itself. That last connection works via the Fisher metric, though that story lies beyond this article. This article builds Fisher information from first principles. We define the score, and establish its mean-zero property under regularity conditions. We define Fisher information as its variance. We then prove the crucial identity relating information to the curvature (second derivative) of the log-likelihood. We work carefully through the regularity conditions that make differentiation under the integral sign legitimate. This is exactly where the theory can silently fail. By the end, you will be equipped to compute Fisher information for standard families. You will also learn to recognize when the standard regularity conditions break down. Finally, you will see how this machinery feeds directly into the Cramer-Rao Lower Bound. It also feeds into the asymptotic theory of MLEs — the natural next stops after this one.

Key takeaways
  • The score is U(θ)=∂θlog⁡f(X;θ)U(\theta) = \partial_\theta \log f(X;\theta), the sensitivity of the log-likelihood to the parameter.
  • Under regularity conditions, the score has mean zero: Eθ[U(θ)]=0\mathbb{E}_\theta[U(\theta)] = 0.
  • Fisher information I(θ)=Var⁡θ(U(θ))=Eθ[U(θ)2]I(\theta) = \operatorname{Var}_\theta(U(\theta)) = \mathbb{E}_\theta[U(\theta)^2] measures how much one observation reveals about θ\theta.
  • An equivalent, often easier formula: I(θ)=−Eθ[∂θ2log⁡f(X;θ)]I(\theta) = -\mathbb{E}_\theta\big[\partial_\theta^2 \log f(X;\theta)\big], linking information to log-likelihood curvature.
  • For nn i.i.d. observations, information is additive: In(θ)=n I(θ)I_n(\theta) = n\, I(\theta).
  • Key idea: Fisher information quantifies the average curvature of the log-likelihood, and hence the precision achievable by likelihood-based inference.

Where this lives today

Fisher information is the load-bearing quantity of classical statistical inference. It appears directly in the Cramer-Rao Lower Bound, which states that no unbiased estimator can have variance smaller than 1/In(θ)1/I_n(\theta) — turning the information computed here into a hard performance guarantee. It governs the asymptotic variance of the maximum likelihood estimator: under regularity, n(θ^n−θ)→N(0,I(θ)−1)\sqrt n(\hat\theta_n - \theta) \to N(0, I(\theta)^{-1}), so Fisher information directly predicts the width of confidence intervals built from likelihood theory (see Properties of MLEs). Likelihood-ratio, Wald, and score (Rao) tests in applied statistics all use estimates of I(θ)I(\theta) to build test statistics and standard errors reported by every generalized linear model fitting routine. Beyond classical statistics, Fisher information equips the parameter space of a statistical model with a Riemannian metric — the Fisher information metric — the starting point of information geometry, connecting statistics to differential geometry. In physics, the same quantity appears in quantum estimation theory (quantum Fisher information bounds the precision of parameter estimation from quantum measurements) and in statistical mechanics via its close relationship to relative entropy. In signal processing and communications engineering, Fisher information underlies the Cramér–Rao bound used to assess the fundamental accuracy limits of radar, sonar, and localization systems. In cryptography and information theory, Fisher information's local, "small perturbation" character complements Shannon entropy's global characterization of uncertainty, and both concepts intersect in the study of the relationship between statistical estimation and channel capacity.

:::quiz[Under the regularity conditions of the theorem, what is Eθ[U(θ;X)]\mathbb{E}_\theta[U(\theta;X)]?]

  • I(θ)I(\theta)
  • 11
  • −I(θ)-I(\theta)
  • 00 ✓

:::faq[Why does the sign convention in I(θ)=−Eθ[∂θ2log⁡f]I(\theta) = -\mathbb{E}_\theta[\partial_\theta^2 \log f] make sense?] Because the log-likelihood attains a local maximum at the true parameter value (in a well-behaved model, on average), its second derivative there is typically negative — the log-likelihood curves downward from its peak. Negating this negative curvature yields a positive number, matching the fact that I(θ)I(\theta) is a variance and therefore must be nonnegative. Large negative curvature (a sharply peaked log-likelihood) corresponds to large Fisher information and precise estimation; near-zero curvature (a flat log-likelihood) corresponds to small Fisher information and imprecise estimation, exactly matching the intuition built in the overview.

Ask the tutor: How does Fisher information generalize to a vector parameter, and what does the resulting Fisher information matrix look like for the normal distribution with both mean and variance unknown?

DefinitionScore function and Fisher information

Let {f(⋅;θ):θ∈Θ}\{f(\cdot;\theta) : \theta \in \Theta\}, Θ⊆R\Theta \subseteq \mathbb{R} an open interval, be a family of probability density (or mass) functions for a random variable XX, all sharing a common support that does not depend on θ\theta. Assume:

(R1) For each xx, θ↦f(x;θ)\theta \mapsto f(x;\theta) is differentiable on Θ\Theta, and for each θ\theta, ∫f(x;θ) dx=1\int f(x;\theta)\,dx = 1 may be differentiated under the integral sign:

ddθ∫f(x;θ) dx=∫∂∂θf(x;θ) dx.\frac{d}{d\theta}\int f(x;\theta)\,dx = \int \frac{\partial}{\partial\theta} f(x;\theta)\,dx.

(R2) f(x;θ)>0f(x;\theta) > 0 on a common support independent of θ\theta, so that log⁡f(x;θ)\log f(x;\theta) is well defined wherever f(x;θ)f(x;\theta) is evaluated. The score function is

U(θ;x)=∂∂θlog⁡f(x;θ)=∂f(x;θ)/∂θf(x;θ).U(\theta; x) = \frac{\partial}{\partial \theta} \log f(x;\theta) = \frac{\partial f(x;\theta)/\partial\theta}{f(x;\theta)}.

Evaluated at the random variable X∼f(⋅;θ)X \sim f(\cdot;\theta), U(θ;X)U(\theta;X) is a random variable, the score statistic. The Fisher information in a single observation is

I(θ)=Var⁡θ(U(θ;X))=Eθ[U(θ;X)2],I(\theta) = \operatorname{Var}_\theta\big(U(\theta;X)\big) = \mathbb{E}_\theta\big[U(\theta;X)^2\big],

the second equality holding whenever Eθ[U(θ;X)]=0\mathbb{E}_\theta[U(\theta;X)] = 0 (established in the Theorem below). For a sample X1,…,XnX_1,\dots,X_n i.i.d. from f(⋅;θ)f(\cdot;\theta), the total score is Un(θ)=∑i=1nU(θ;Xi)U_n(\theta) = \sum_{i=1}^n U(\theta;X_i), and the Fisher information in the sample is In(θ)=Var⁡θ(Un(θ))I_n(\theta) = \operatorname{Var}_\theta(U_n(\theta)).

Intuition

Think of the log-likelihood ℓ(θ)=log⁡f(x;θ)\ell(\theta) = \log f(x;\theta) as a hill whose shape depends on the observed data xx. The score U(θ;x)=ℓ′(θ)U(\theta;x) = \ell'(\theta) is the slope of this hill at a given θ\theta. The maximum likelihood estimate is the point where the slope is zero — the summit. Fisher information asks: on average, how sharply peaked is this hill near the true parameter? A large Fisher information means the log-likelihood is sharply curved: nearby values of θ\theta produce very different likelihoods, so the data can distinguish them easily, and the MLE will be precise. A small Fisher information means the log-likelihood is nearly flat: many values of θ\theta explain the data almost equally well, and the MLE will be imprecise. This is why I(θ)I(\theta) enters as the variance of the score (a measure of typical fluctuation of the slope around its zero mean) and, equivalently, as the negative expected curvature (a direct measure of peakedness). The picture below shows two log-likelihood shapes from the same sample size but different underlying models: a peaked one (high information, precise inference) and a flat one (low information, imprecise inference).

Figure
Two log-likelihoods: sharp curvature (high information) vs. flat curvature (low information)
θ ℓ(θ) high I(θ), sharp peak low I(θ), flat peak θ̂ (sharp) θ̂ (flat)

The central theorem

TheoremMean-zero score and the information identity

Let {f(⋅;θ):θ∈Θ}\{f(\cdot;\theta):\theta\in\Theta\} satisfy (R1) and (R2) above, together with:

(R3) For each θ\theta, θ↦f(x;θ)\theta \mapsto f(x;\theta) is twice differentiable, and differentiation under the integral sign is valid also for the second derivative:

d2dθ2∫f(x;θ) dx=∫∂2∂θ2f(x;θ) dx.\frac{d^2}{d\theta^2}\int f(x;\theta)\,dx = \int \frac{\partial^2}{\partial\theta^2} f(x;\theta)\,dx.

(R4) I(θ)=Eθ[U(θ;X)2]<∞I(\theta) = \mathbb{E}_\theta[U(\theta;X)^2] < \infty for all θ∈Θ\theta \in \Theta. Then, for every θ∈Θ\theta \in \Theta:

(a) Mean-zero score:

Eθ[U(θ;X)]=0.\mathbb{E}_\theta\big[U(\theta;X)\big] = 0.

(b) Information identity:

I(θ)=Var⁡θ(U(θ;X))=− Eθ[∂2∂θ2log⁡f(X;θ)].I(\theta) = \operatorname{Var}_\theta\big(U(\theta;X)\big) = -\, \mathbb{E}_\theta\left[\frac{\partial^2}{\partial\theta^2}\log f(X;\theta)\right].

(c) Additivity over i.i.d. samples: if X1,…,XnX_1,\dots,X_n are i.i.d. ∼f(⋅;θ)\sim f(\cdot;\theta), then

In(θ)=n I(θ).I_n(\theta) = n\,I(\theta).
Proof

We prove (a), (b), (c) in turn, using differentiation under the integral sign as the core technique, justified by (R1) and (R3).

Part (a). Since f(⋅;θ)f(\cdot;\theta) is a density (or p.m.f.) on the common support X\mathcal{X},

∫Xf(x;θ) dx=1for all θ.\int_{\mathcal X} f(x;\theta)\,dx = 1 \quad \text{for all } \theta.

Differentiate both sides with respect to θ\theta. The right side has derivative 00. By hypothesis (R1), we may differentiate under the integral sign on the left side:

0=ddθ∫Xf(x;θ) dx=∫X∂∂θf(x;θ) dx.0 = \frac{d}{d\theta}\int_{\mathcal X} f(x;\theta)\,dx = \int_{\mathcal X} \frac{\partial}{\partial\theta} f(x;\theta)\,dx.

Now write the integrand using the identity ∂∂θf(x;θ)=f(x;θ)⋅U(θ;x)\dfrac{\partial}{\partial\theta} f(x;\theta) = f(x;\theta)\cdot U(\theta;x), valid wherever f(x;θ)>0f(x;\theta)>0 by (R2) and the chain rule applied to log⁡f\log f:

0=∫Xf(x;θ) U(θ;x) dx=Eθ[U(θ;X)].0 = \int_{\mathcal X} f(x;\theta)\, U(\theta;x)\, dx = \mathbb{E}_\theta\big[U(\theta;X)\big].

This proves (a). (Note: this is the step where "common support independent of θ\theta" is essential — see the counterexample below for what fails without it.)

Part (b). Because Eθ[U(θ;X)]=0\mathbb{E}_\theta[U(\theta;X)] = 0 by part (a), the definition of Fisher information as a variance coincides with the second-moment formula:

I(θ)=Var⁡θ(U(θ;X))=Eθ[U(θ;X)2]−(Eθ[U(θ;X)])2=Eθ[U(θ;X)2].I(\theta) = \operatorname{Var}_\theta(U(\theta;X)) = \mathbb{E}_\theta[U(\theta;X)^2] - \big(\mathbb{E}_\theta[U(\theta;X)]\big)^2 = \mathbb{E}_\theta[U(\theta;X)^2].

This establishes the second equality claimed in the definition and confirms I(θ)I(\theta) is well defined by (R4). We now derive the curvature formula. Differentiate the identity ∫f(x;θ)U(θ;x) dx=0\int f(x;\theta)U(\theta;x)\,dx = 0 (established in part (a)) once more with respect to θ\theta. By (R3), we may again differentiate under the integral sign:

0=ddθ∫Xf(x;θ) U(θ;x) dx=∫X∂∂θ[f(x;θ) U(θ;x)]dx.0 = \frac{d}{d\theta}\int_{\mathcal X} f(x;\theta)\, U(\theta;x)\, dx = \int_{\mathcal X} \frac{\partial}{\partial\theta}\Big[ f(x;\theta)\, U(\theta;x)\Big] dx.

Apply the product rule inside the integral:

∂∂θ[f(x;θ)U(θ;x)]=∂f(x;θ)∂θ U(θ;x)+f(x;θ) ∂U(θ;x)∂θ.\frac{\partial}{\partial\theta}\Big[f(x;\theta)U(\theta;x)\Big] = \frac{\partial f(x;\theta)}{\partial\theta}\, U(\theta;x) + f(x;\theta)\, \frac{\partial U(\theta;x)}{\partial\theta}.

Using ∂θf(x;θ)=f(x;θ)U(θ;x)\partial_\theta f(x;\theta) = f(x;\theta) U(\theta;x) again in the first term, and noting ∂θU(θ;x)=∂θ2log⁡f(x;θ)\partial_\theta U(\theta;x) = \partial_\theta^2 \log f(x;\theta) by definition of the score, we get

0=∫Xf(x;θ) U(θ;x)2 dx  +  ∫Xf(x;θ) ∂2∂θ2log⁡f(x;θ) dx.0 = \int_{\mathcal X} f(x;\theta)\, U(\theta;x)^2\, dx \;+\; \int_{\mathcal X} f(x;\theta)\, \frac{\partial^2}{\partial\theta^2}\log f(x;\theta)\, dx.

The first integral is exactly Eθ[U(θ;X)2]=I(θ)\mathbb{E}_\theta[U(\theta;X)^2] = I(\theta) from the computation above. The second integral is Eθ[∂θ2log⁡f(X;θ)]\mathbb{E}_\theta\big[\partial_\theta^2 \log f(X;\theta)\big]. Hence

0=I(θ)+Eθ[∂2∂θ2log⁡f(X;θ)],0 = I(\theta) + \mathbb{E}_\theta\left[\frac{\partial^2}{\partial\theta^2}\log f(X;\theta)\right],

which rearranges to the claimed identity:

I(θ)=− Eθ[∂2∂θ2log⁡f(X;θ)].I(\theta) = -\,\mathbb{E}_\theta\left[\frac{\partial^2}{\partial\theta^2}\log f(X;\theta)\right].

Part (c). Let ℓn(θ)=∑i=1nlog⁡f(Xi;θ)\ell_n(\theta) = \sum_{i=1}^n \log f(X_i;\theta) be the log-likelihood of the sample, so the total score is Un(θ)=∑i=1nU(θ;Xi)U_n(\theta) = \sum_{i=1}^n U(\theta;X_i), a sum of i.i.d. random variables (since the XiX_i are i.i.d., each U(θ;Xi)U(\theta;X_i) has the same distribution as U(θ;X)U(\theta;X)). Variance of a sum of independent random variables equals the sum of variances:

In(θ)=Var⁡θ(Un(θ))=∑i=1nVar⁡θ(U(θ;Xi))=∑i=1nI(θ)=n I(θ).I_n(\theta) = \operatorname{Var}_\theta(U_n(\theta)) = \sum_{i=1}^n \operatorname{Var}_\theta(U(\theta;X_i)) = \sum_{i=1}^n I(\theta) = n\,I(\theta).

This uses only independence (not identical distribution) for the variance-additivity step, and identical distribution to replace each term by the common value I(θ)I(\theta). ■\blacksquare

∎

Worked examples

Example 1: Exponential distribution (asymmetric rate parameterization). Let X∼Exp(θ)X \sim \mathrm{Exp}(\theta) with density f(x;θ)=θe−θxf(x;\theta) = \theta e^{-\theta x} for x>0x > 0, θ>0\theta > 0. We verify the regularity conditions hold (the support (0,∞)(0,\infty) does not depend on θ\theta, and ff is smooth in θ\theta with integrable derivatives — a routine dominated-convergence check we take as given here), then compute I(θ)I(\theta) two ways. Log-likelihood and score.

log⁡f(x;θ)=log⁡θ−θx,U(θ;x)=1θ−x.\log f(x;\theta) = \log\theta - \theta x, \qquad U(\theta;x) = \frac{1}{\theta} - x.

Check mean-zero score. Since Eθ[X]=1/θ\mathbb{E}_\theta[X] = 1/\theta,

Eθ[U(θ;X)]=1θ−Eθ[X]=1θ−1θ=0,\mathbb{E}_\theta[U(\theta;X)] = \frac{1}{\theta} - \mathbb{E}_\theta[X] = \frac{1}{\theta} - \frac{1}{\theta} = 0,

confirming part (a) of the theorem directly. Fisher information via variance of the score. Since U(θ;X)=1θ−XU(\theta;X) = \tfrac1\theta - X, Var⁡θ(U(θ;X))=Var⁡θ(X)\operatorname{Var}_\theta(U(\theta;X)) = \operatorname{Var}_\theta(X). For Exp(θ)\mathrm{Exp}(\theta), Var⁡θ(X)=1/θ2\operatorname{Var}_\theta(X) = 1/\theta^2. Hence

I(θ)=1θ2.I(\theta) = \frac{1}{\theta^2}.

Fisher information via curvature (cross-check). Differentiate the score:

∂U∂θ=∂2∂θ2log⁡f(x;θ)=−1θ2.\frac{\partial U}{\partial\theta} = \frac{\partial^2}{\partial\theta^2}\log f(x;\theta) = -\frac{1}{\theta^2}.

This does not depend on xx, so

I(θ)=−Eθ[−1θ2]=1θ2,I(\theta) = -\mathbb{E}_\theta\left[-\frac{1}{\theta^2}\right] = \frac{1}{\theta^2},

matching the direct computation exactly, as guaranteed by part (b) of the theorem. Sample of size nn. For nn i.i.d. exponential observations, In(θ)=n/θ2I_n(\theta) = n/\theta^2, consistent with additivity (part (c)). This number will reappear as the denominator in the Cramér–Rao bound for estimating θ\theta: any unbiased estimator of θ\theta has variance at least θ2/n\theta^2/n.

Example 2: Poisson distribution with a nonstandard target (information about λ2\lambda^2, illustrating reparametrization pitfalls). Let X∼Poisson(λ)X \sim \mathrm{Poisson}(\lambda), λ>0\lambda > 0, with p.m.f. f(x;λ)=λxe−λx!f(x;\lambda) = \dfrac{\lambda^x e^{-\lambda}}{x!}, x=0,1,2,…x = 0,1,2,\dots. Score and information in λ\lambda.

log⁡f(x;λ)=xlog⁡λ−λ−log⁡(x!),U(λ;x)=xλ−1.\log f(x;\lambda) = x\log\lambda - \lambda - \log(x!), \qquad U(\lambda;x) = \frac{x}{\lambda} - 1.

Mean-zero check: Eλ[X]=λ\mathbb{E}_\lambda[X] = \lambda, so Eλ[U(λ;X)]=λ/λ−1=0\mathbb{E}_\lambda[U(\lambda;X)] = \lambda/\lambda - 1 = 0. Good. Variance of the score: Var⁡λ(U(λ;X))=Var⁡λ(X)/λ2=λ/λ2=1/λ\operatorname{Var}_\lambda(U(\lambda;X)) = \operatorname{Var}_\lambda(X)/\lambda^2 = \lambda/\lambda^2 = 1/\lambda. Curvature check: ∂λU=−x/λ2\partial_\lambda U = -x/\lambda^2, so I(λ)=−Eλ[−X/λ2]=λ/λ2=1/λI(\lambda) = -\mathbb{E}_\lambda[-X/\lambda^2] = \lambda/\lambda^2 = 1/\lambda. Both agree: I(λ)=1/λI(\lambda) = 1/\lambda. Now suppose we instead parameterize by η=λ2\eta = \lambda^2 and ask for the information about η\eta, illustrating that Fisher information is <strong>not</strong> parameterization-invariant in absolute terms — it transforms. Write λ=η\lambda = \sqrt{\eta}, so the density as a function of η\eta is g(x;η)=f(x;η)g(x;\eta) = f(x;\sqrt\eta), and

log⁡g(x;η)=xlog⁡η−η−log⁡(x!)=x2log⁡η−η−log⁡(x!).\log g(x;\eta) = x\log\sqrt\eta - \sqrt\eta - \log(x!) = \tfrac{x}{2}\log\eta - \sqrt\eta - \log(x!).

The score in η\eta is

Uη(η;x)=x2η−12η.U_\eta(\eta;x) = \frac{x}{2\eta} - \frac{1}{2\sqrt\eta}.

Its variance is Var⁡η(X)/(4η2)=λ/(4η2)=η/(4η2)=1/(4η3/2)\operatorname{Var}_\eta(X)/(4\eta^2) = \lambda/(4\eta^2) = \sqrt\eta/(4\eta^2) = 1/(4\eta^{3/2}). Substituting η=λ2\eta = \lambda^2 gives I(η)=1/(4λ3)I(\eta) = 1/(4\lambda^3). Sanity check via the change-of-variables rule I(η)=I(λ)(dλdη)2I(\eta) = I(\lambda)\left(\dfrac{d\lambda}{d\eta}\right)^2 (a consequence of the chain rule applied to the score, provable directly from the definition): with λ=η\lambda = \sqrt\eta, dλ/dη=12η=12λd\lambda/d\eta = \tfrac{1}{2\sqrt\eta} = \tfrac{1}{2\lambda}, so

I(η)=1λ⋅14λ2=14λ3,I(\eta) = \frac{1}{\lambda}\cdot \frac{1}{4\lambda^2} = \frac{1}{4\lambda^3},

matching. This example shows numerically that Fisher information depends on the chosen parameterization — a subtlety often glossed over, and one reason the Cramér–Rao bound must always be quoted with the parameter it is measuring information about.

CounterexampleWhy the "common support" hypothesis is essential

Drop hypothesis (R2)'s requirement that the support of f(⋅;θ)f(\cdot;\theta) not depend on θ\theta, keeping everything else. Consider the Uniform(0,θ)\mathrm{Uniform}(0,\theta) family, θ>0\theta > 0:

f(x;θ)=1θ 1{0<x<θ}.f(x;\theta) = \frac{1}{\theta}\, \mathbf 1\{0 < x < \theta\}.

Formally differentiating log⁡f(x;θ)=−log⁡θ\log f(x;\theta) = -\log\theta (for 0<x<θ0<x<\theta) with respect to θ\theta gives the "score"

U(θ;x)  "= ⁣"  −1θ,U(\theta;x) \;"=\!"\; -\frac{1}{\theta},

which is a constant (not even random), so naively

Eθ[U(θ;X)]=−1θ≠0.\mathbb{E}_\theta[U(\theta;X)] = -\frac{1}{\theta} \neq 0.

This directly contradicts part (a) of the theorem. The reason the proof breaks: the key step

ddθ∫0θf(x;θ) dx=∫0θ∂∂θf(x;θ) dx\frac{d}{d\theta}\int_0^\theta f(x;\theta)\,dx = \int_0^\theta \frac{\partial}{\partial\theta}f(x;\theta)\,dx

is false here, because the limits of integration depend on θ\theta. By Leibniz's rule for differentiating an integral with variable limits,

ddθ∫0θ1θ dx=ddθ(1)=0,\frac{d}{d\theta}\int_0^{\theta} \frac{1}{\theta}\,dx = \frac{d}{d\theta}(1) = 0,

but the naive "differentiate the integrand only" computation gives

∫0θ∂∂θ(1θ)dx=∫0θ(−1θ2)dx=−1θ≠0.\int_0^\theta \frac{\partial}{\partial\theta}\left(\frac1\theta\right)dx = \int_0^\theta \left(-\frac{1}{\theta^2}\right)dx = -\frac1\theta \ne 0.

The extra boundary term from Leibniz's rule, f(θ;θ)⋅1=1θf(\theta;\theta)\cdot 1 = \tfrac1\theta, exactly cancels this discrepancy: −1θ+1θ=0-\tfrac1\theta + \tfrac1\theta = 0, confirming the true derivative is 00, not −1/θ-1/\theta. So (R1) fails precisely because of the θ\theta-dependent support, hypothesis (R2) is violated, and the mean-zero score property — hence the entire information machinery — collapses. Fisher information is simply not the right tool for this model; the MLE θ^=X(n)\hat\theta = X_{(n)} (the sample maximum) in fact converges at rate nn, not n\sqrt n, a signature of irregular models where the standard theory does not apply.

Scope, edge cases & common traps

SituationWhat happensWhy
Regular family (R1–R4 hold)I(θ)I(\theta) well defined, both formulas agreeTheorem above
θ\theta-dependent support (e.g. Uniform(0,θ)\mathrm{Uniform}(0,\theta))Score not mean-zero; I(θ)I(\theta) formula invalidDifferentiation under the integral sign fails (counterexample)
Reparameterization θ→η=g(θ)\theta \to \eta=g(\theta)I(η)=I(θ) (dθ/dη)2I(\eta) = I(\theta)\,(d\theta/d\eta)^2Chain rule on the score; information is not invariant, it transforms as a "density"
Multiple parameters θ∈Rk\boldsymbol\theta \in \mathbb{R}^kInformation becomes a k×kk\times k Fisher information matrixSame construction applied to the gradient of the log-likelihood
Discontinuous or non-differentiable f(x;θ)f(x;\theta) in θ\thetaScore undefined at those points; need care or a different framework(R1) presupposes differentiability
Non i.i.d. data (e.g. dependent observations)Additivity In=nII_n = nI fails in generalProof of part (c) used independence explicitly

The mathematician behind it

Origins · 1 minRonald Aylmer Fisher and how this was discovered
RA
Ronald Aylmer Fisher
1890–1962 · Statistics, genetics, and evolutionary biology, Cambridge and Rothamsted Experimental Station

Fisher developed the concepts of maximum likelihood, sufficiency, and information for parameters in a sequence of papers in the 1920s, most notably On the Mathematical Foundations of Theoretical Statistics (1922) and Theory of Statistical Estimation (1925). He was simultaneously a founder of modern population genetics (co-founding, with Sewall Wright and J.B.S. Haldane, the field's mathematical foundations) and the designer of experimental methods — randomization, blocking, analysis of variance — still standard in agricultural and clinical trials today. His concept of "information" formalized an intuition already implicit in the geometry of maximum likelihood: that the curvature of the likelihood surface measures the precision attainable from data.

History
- 1912 — Fisher, as an undergraduate, proposes an early version of maximum likelihood estimation.
- 1922 — On the Mathematical Foundations of Theoretical Statistics introduces "likelihood" and lays groundwork for information as a curvature concept.
- 1925 — Theory of Statistical Estimation formally names and develops "the amount of information" carried by an observation.
- 1945–1946 — Harald Cramér and C.R. Rao independently derive the variance lower bound now named after them, built directly on Fisher information.
- 1950s onward — Fisher information becomes the organizing quantity for asymptotic efficiency theory of MLEs, and later for Fisher's information metric in information geometry.
Why is Fisher information defined as a variance rather than, say, an expectation of the score?

Because the expectation of the score is always zero under regularity (this is proven, not assumed), so it carries no information about the model — every regular family has mean-zero score regardless of how informative the data is. The spread of the score around its mean of zero, however, does distinguish informative models from uninformative ones: a score that is usually far from zero indicates the log-likelihood's slope is highly sensitive to small changes in the data, meaning different values of θ\theta produce visibly different likelihoods. Variance is the natural way to quantify that spread, and it turns out (via the curvature identity) to coincide exactly with the negative expected second derivative of the log-likelihood, giving a second, geometrically intuitive interpretation.

Does Fisher information always exist and stay finite?

No. Existence requires hypothesis (R4), that Eθ[U(θ;X)2]<∞\mathbb{E}_\theta[U(\theta;X)^2] < \infty, plus the differentiability and interchange conditions (R1)–(R3). Some perfectly reasonable-looking families violate these: distributions with θ\theta-dependent support (like Uniform(0,θ)\mathrm{Uniform}(0,\theta)) fail even the mean-zero score property, and some heavy-tailed families can have an infinite second moment of the score. When Fisher information fails to exist or be finite, the entire asymptotic theory built on it — the Cramér–Rao bound, the asymptotic normality of MLEs with variance 1/I(θ)1/I(\theta) — needs separate, non-standard treatment.

Is Fisher information the same as Shannon information entropy?

No, though both are called "information" and both originate in early-to-mid 20th century mathematics. Shannon entropy H(X)=−E[log⁡f(X)]H(X) = -\mathbb{E}[\log f(X)] measures the average "surprise" or uncertainty in a random variable's own distribution, with no reference to an unknown parameter to be estimated. Fisher information I(θ)=Eθ[U(θ;X)2]I(\theta) = \mathbb{E}_\theta[U(\theta;X)^2] measures how sensitive the distribution is to a parameter, and hence how estimable that parameter is. They are related — e.g., Fisher information appears as the local curvature of relative entropy (KL divergence) between nearby members of a parametric family — but they answer fundamentally different questions.

How do I compute Fisher information in practice: via the variance formula or the curvature formula?

Whichever is algebraically easier for the family at hand — the theorem guarantees they agree under regularity. For densities where log⁡f(x;θ)\log f(x;\theta) is a simple polynomial or linear function of a sufficient statistic (exponential families in canonical form), the curvature formula −Eθ[∂θ2log⁡f]-\mathbb{E}_\theta[\partial_\theta^2 \log f] is usually fastest, because the second derivative often doesn't depend on xx at all (as in the exponential example above), turning the expectation into a triviality. When the second derivative is messy but the score itself is a simple linear function of XX, computing Var⁡θ(U(θ;X))\operatorname{Var}_\theta(U(\theta;X)) directly from known moments of XX (as in both worked examples) is often faster.

Does Fisher information depend on the sample size, or is it a property of a single observation?

Fisher information as originally defined, I(θ)I(\theta), is a property of a single observation's density. When you have nn i.i.d. observations, the total information in the sample, In(θ)I_n(\theta), scales linearly: In(θ)=n I(θ)I_n(\theta) = n\,I(\theta), proven directly from independence in part (c) of the theorem. This additivity is what drives the n\sqrt n rate of convergence in the asymptotic normality of maximum likelihood estimators: the estimator's asymptotic variance is 1/In(θ)=1/(nI(θ))1/I_n(\theta) = 1/(nI(\theta)), shrinking at rate 1/n1/n.

What goes wrong if I use Fisher information for a model with a discrete parameter or with parameters restricted to a boundary?

The entire construction assumes Θ\Theta is an open interval so that derivatives with respect to θ\theta make sense in a neighborhood of every point, including the true parameter value. If θ\theta lives on a boundary of the parameter space (e.g., a variance component constrained to be ≥0\ge 0, with the true value equal to 00), one-sided derivatives replace two-sided ones, and the standard asymptotic theory built on Fisher information (the Cramér–Rao bound, asymptotic normality of the MLE) needs substantial modification. This is a genuinely different, non-regular regime and is a common trap in variance-component and mixture models.

Before this

Where this leads