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Optimal Bonus-Malus Relativities


Proposition

For random claim rate Λ\Lambda and stationary class LL, the unconstrained class value rlr_l minimizing E[(Λ−rL)2]\mathbb{E}[(\Lambda-r_L)^2] is rl=E[Λ∣L=l]r_l=\mathbb{E}[\Lambda\mid L=l], for classes of positive probability and finite second moments. This is on a claim-frequency scale; dimensionless premium relativities require normalization by a base rate.


Interpretation

Each class is priced by the average underlying rate among its members. This minimizes squared prediction error, but can produce an irregular or commercially unsuitable scale.

Bar chart of two equally frequent bonus-malus classes with conditional rates 0.1 and 0.3, a dashed base-rate line at 0.2, and a right axis rescaling them to relativities 0.5 and 1.5.

The figure draws the example below: two equally frequent classes whose members have average claim rates E[Λ∣L=1]=0.1\mathbb{E}[\Lambda\mid L=1]=0.1 and E[Λ∣L=2]=0.3\mathbb{E}[\Lambda\mid L=2]=0.3. These are the optimal class values on the claim-frequency scale (left axis). Their probability-weighted average is 12(0.1)+12(0.3)=0.2=E[Λ]\tfrac{1}{2}(0.1)+\tfrac{1}{2}(0.3)=0.2=\mathbb{E}[\Lambda], in line with E[rL]=E[Λ]\mathbb{E}[r_L]=\mathbb{E}[\Lambda]; dividing by this base rate gives the dimensionless relativities 0.50.5 and 1.51.5 on the right axis.

The stationary bonus-malus distribution and premium supplies the long-run class probabilities used to weight claim rates within each class. Conditional expectation given a random variable minimizes squared prediction error within that class, giving rl=E[Λ∣L=l]r_l=\mathbb{E}[\Lambda\mid L=l]. Under a linear restriction, covariance measures the joint variation of risk and class, while variance and standard deviation supplies the class spread in the denominator of the regression slope.


Key Results

  • If class probability at fixed rate is πl(λ)\pi_l(\lambda) and rate density is fΛf_\Lambda, then rl=∫λπl(λ)fΛ(λ) dλ/∫πl(λ)fΛ(λ) dλr_l=\int\lambda\pi_l(\lambda)f_\Lambda(\lambda)\,\mathrm{d}\lambda/\int\pi_l(\lambda)f_\Lambda(\lambda)\,\mathrm{d}\lambda.
  • E[rL]=E[Λ]\mathbb{E}[r_L]=\mathbb{E}[\Lambda].
  • Under a linear restriction rl=a+blr_l=a+bl and Var⁡(L)>0\operatorname{Var}(L)>0, b=Cov⁡(Λ,L)/Var⁡(L)b=\operatorname{Cov}(\Lambda,L)/\operatorname{Var}(L) and a=E[Λ]−bE[L]a=\mathbb{E}[\Lambda]-b\mathbb{E}[L].
  • Refining the same information partition cannot increase unconstrained minimum mean squared error (MSE). Merely changing the number of classes in a different system does not guarantee an improvement.

Examples

If two equally frequent classes have conditional rates 0.1 and 0.3, their optimal frequency-scale values are 0.1 and 0.3. At base rate 0.2, the dimensionless relativities are 0.5 and 1.5.


Prerequisites



Sources

Aliases: minimum-MSE BMS scale, linear premium relativities, optimal relativities, optimal premium relativities Keywords: r_l = E[Λ | L = l], mean squared error, b = Cov(Λ, L)/Var(L), normalization by a base rate Symbols: integral, lambda, pi

Last updated: 14 October 2026 08:21