St · Statistics & Probability

What Is the Fisher Information of the Rayleigh Distribution?

Updated 13 October 2026

At a glance

  1. 1. Set the parameterization

    Use the scale parameter sigma in the standard Rayleigh density, and note that other parameterizations give different formulas.

  2. 2. Write the log-likelihood

    Take the logarithm of the density for one observation and differentiate with respect to sigma.

  3. 3. Take the expectation

    Use the Rayleigh moment E[X squared] = 2 sigma squared to find the expected negative second derivative.

  4. 4. Extend to a sample

    For n independent observations, multiply the one-observation information by n.

The Fisher information of a Rayleigh distribution depends on which parameter you use. With the common scale parameterization, the density is f(x;σ)=xσ2exp⁡(−x22σ2)f(x;\sigma)=\frac{x}{\sigma^2}\exp\left(-\frac{x^2}{2\sigma^2}\right) for x≥0x\geq 0 and σ>0\sigma>0. In this parameterization, one observation contains 4/σ24/\sigma^2 units of Fisher information about σ\sigma.

For nn independent observations, information adds, giving 4n/σ24n/\sigma^2. The alternative parameter θ=σ2\theta=\sigma^2 is also common; its information is 1/θ21/\theta^2 per observation. The derivation below shows where these results come from and how to avoid mixing the parameterizations.

Fisher information for the scale parameter

For a density f(x;σ)f(x;\sigma), the Fisher information in one observation can be calculated as either the variance of the score or the expected negative second derivative of the log-density:

I(σ)=E[(∂∂σlog⁡f(X;σ))2]=−E[∂2∂σ2log⁡f(X;σ)].I(\sigma)=\mathbb{E}\left[\left(\frac{\partial}{\partial\sigma}\log f(X;\sigma)\right)^2\right]=-\mathbb{E}\left[\frac{\partial^2}{\partial\sigma^2}\log f(X;\sigma)\right].

These two formulas agree under the usual regularity conditions. For the Rayleigh scale family, the support x≥0x\geq 0 does not depend on σ\sigma, so the standard calculation applies.

For one observation XX, take the logarithm of the density:

ℓ(σ;x)=log⁡x−2log⁡σ−x22σ2.\ell(\sigma;x)=\log x-2\log\sigma-\frac{x^2}{2\sigma^2}.

Differentiate once to get the score, and again to get the second derivative:

∂ℓ∂σ=−2σ+x2σ3,∂2ℓ∂σ2=2σ2−3x2σ4.\frac{\partial\ell}{\partial\sigma}=-\frac{2}{\sigma}+\frac{x^2}{\sigma^3},\qquad \frac{\partial^2\ell}{\partial\sigma^2}=\frac{2}{\sigma^2}-\frac{3x^2}{\sigma^4}.

The Rayleigh second moment is E[X2]=2σ2\mathbb{E}[X^2]=2\sigma^2. Substituting it into the expected negative second derivative gives

I(σ)=−E[2σ2−3X2σ4]=−2σ2+3(2σ2)σ4=4σ2.\begin{aligned} I(\sigma)&=-\mathbb{E}\left[\frac{2}{\sigma^2}-\frac{3X^2}{\sigma^4}\right]\\ &=-\frac{2}{\sigma^2}+\frac{3(2\sigma^2)}{\sigma^4}\\ &=\frac{4}{\sigma^2}. \end{aligned}

Thus, for one Rayleigh observation parameterized by its scale σ\sigma, the Fisher information is 4/σ24/\sigma^2.

Check using the score variance

The score is U(σ;X)=−2/σ+X2/σ3U(\sigma;X)=-2/\sigma+X^2/\sigma^3. Its expected value is zero because E[X2]=2σ2\mathbb{E}[X^2]=2\sigma^2. Also, the fourth moment is E[X4]=8σ4\mathbb{E}[X^4]=8\sigma^4, so

Var⁡(X2)=8σ4−(2σ2)2=4σ4.\operatorname{Var}(X^2)=8\sigma^4-(2\sigma^2)^2=4\sigma^4.

The constant term in the score does not affect its variance, hence

Var⁡(U)=Var⁡(X2)σ6=4σ2,\operatorname{Var}(U)=\frac{\operatorname{Var}(X^2)}{\sigma^6}=\frac{4}{\sigma^2},

which confirms the result.

Information in a sample of size n

If X1,…,XnX_1,\ldots,X_n are independent Rayleigh observations with the same scale σ\sigma, their log-likelihood is the sum of the individual log-likelihoods. Independent observations contribute additive Fisher information, so

In(σ)=nI(σ)=4nσ2.I_n(\sigma)=nI(\sigma)=\frac{4n}{\sigma^2}.

For example, suppose σ=2\sigma=2 and the sample contains n=10n=10 observations. Then

I10(2)=4(10)22=10.I_{10}(2)=\frac{4(10)}{2^2}=10.

For an unbiased estimator of σ\sigma under the usual regularity conditions, the Cramér–Rao lower bound is therefore Var⁡(σ^)≥1/In(σ)=σ2/(4n)\operatorname{Var}(\hat\sigma)\geq 1/I_n(\sigma)=\sigma^2/(4n). In this numerical example, that bound is 0.10.1.

If the parameter is the squared scale

Some sources write the same family using θ=σ2\theta=\sigma^2:

f(x;θ)=xθexp⁡(−x22θ),θ>0.f(x;\theta)=\frac{x}{\theta}\exp\left(-\frac{x^2}{2\theta}\right),\qquad \theta>0.

The information must be recalculated for this parameter, or transformed using the chain rule. Since dσ/dθ=1/(2θ)d\sigma/d\theta=1/(2\sqrt{\theta}), information transforms as Iθ=Iσ(dσ/dθ)2I_\theta=I_\sigma(d\sigma/d\theta)^2. Therefore,

Iθ=4σ2⋅14θ=1θ2,I_\theta=\frac{4}{\sigma^2}\cdot\frac{1}{4\theta}=\frac{1}{\theta^2},

because σ2=θ\sigma^2=\theta. For nn observations, In(θ)=n/θ2I_n(\theta)=n/\theta^2. The two answers describe the same distribution but refer to different parameters; Fisher information is not unchanged by a change of parameter.

Common mistakes

  • Using a different scale convention. In the standard density above, σ\sigma is the Rayleigh scale and E[X2]=2σ2\mathbb{E}[X^2]=2\sigma^2. Check the density before using a formula from another source.
  • Forgetting to square the score. The score-variance formula uses the expected square of the score, not just its expected value; the score itself has expectation zero.
  • Confusing one observation with a sample. The information for nn independent observations is nn times the single-observation information.
  • Changing parameters without transforming information. The formula 4/σ24/\sigma^2 is for σ\sigma, whereas 1/θ21/\theta^2 is for θ=σ2\theta=\sigma^2.

References

  1. Statistical Inference, George Casella and Roger L. Berger
  2. Theory of Point Estimation, Erich L. Lehmann and George Casella

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