Natural parameter space 2026-10-05
The natural parameter space is the set of for which the normalizing integral is finite. Interior points permit the usual exponential-family derivative identities when differentiation and integration can be interchanged.
Past exam of the mathematics course of the University of Cambridge 2012 iii Paper 40 4 Solution Created 2026-10-03 Updated 2026-10-07
A credibility estimate blends the risk's own sample mean with a population or prior expected value. In the basic equal-exposure form it is , where the credibility factor is the weight attached to the individual experience. More data ordinarily increase that weight; greater within-risk variation relative to between-risk variation reduces it.
Write for the conditional claim expected value, keeping for the prior-level parameter. Normalization of the probability density function givesAt interior points of its finite domain, differentiation under the integral sign yieldsThis is an instance of the exponential-family derivative identities for natural parameter . The minus sign is present in the PDF and is lost in the converted TeX. The conditional variance is likewise .
Differentiate the log of the natural conjugate prior:Integrate on a compact subinterval and then let its endpoints approach those of the parameter interval. The prescribed vanishing of the prior density eliminates the boundary term. Since , monotone convergence theorem justifies the limit of its expectation, and the identity givesIn particular the assumed proper prior and boundary conditions themselves establish this first-moment integrability.
For and , conditional independence makes the likelihood function proportional to . Multiplication by the prior distribution gives the Bayesian posteriorThus this is a conjugate prior family, with updated parameters
The integration-by-parts calculation for the posterior mean also needs vanishing posterior boundary values. Here that property can be checked, rather than assumed. Let be the essential lower and upper endpoints of the claim support. Every nondegenerate tilted claim law has , so the established prior mean satisfies . Supported observations have ; hence . At a finite parameter endpoint the prior's vanishing forces , because its exponential factor has a finite positive limit; the increased power makes the posterior vanish there too. At , choose with positive base-measure mass below . Then and the unnormalized posterior is at most . At , choose with positive mass above to obtain the corresponding bound . These bounds also ensure posterior propriety at infinite endpoints. This is the endpoint control for a Laplace-family conjugate posterior.
Apply the previous score integration to the Bayesian posterior. The natural conjugate credibility identity isThus is the credibility factor. This is an exact posterior mean, rather than an affine approximation to one.
For the specific shape-two gamma distribution, takeThen and . The gamma rate gamma conjugacy prior isthat is, . Its normalizing constant in the notation of the question is . The gamma distribution density vanishes at both zero and infinity for . The posterior has shape and rate , so its conditional-mean posterior mean is again .
For the last calculation, gamma distribution integration givesThe second identity requires the printed . Therefore the expected process variance and variance of hypothetical means, denoted by in this question, areConsequently , and the Bühlmann credibility factor agrees with the exact Bayesian weight:This is the exact Bühlmann credibility for gamma claims, expressed using the reciprocal rate as the random scale. The symbols here are the process and between-risk variances, respectively; their roles should not be interchanged when comparing with other notation for the Bühlmann model.
Past exam of the mathematics course of the University of Cambridge 2014 iii Paper 33 3 a Solution Created 2026-10-03 Updated 2026-10-06
Write and . With , the Gamma exponential dispersion family representation iswhereSubstitution gives the original gamma density, so both unknown parameters are included. The exponential-family derivative identities yield and . ThereforeThe exact natural-parameter canonical link function is . The usual inverse-link convention is , as used by the printed R fits; multiplying the link and coefficients by gives the natural-parameter convention. The sign convention changes neither the fitted means nor the weight matrix below.
Past exam of the mathematics course of the University of Cambridge 2021 ii Paper 1 5J Solution Created 2026-09-24 Updated 2026-09-25
Expand the exponent in the Inverse Gaussian distribution with unit shape parameter:Consequently its probability density function can be written aswhereIndeed, . This is the canonical form of a one-parameter exponential family, and its natural parameter is therefore
Past exam of the mathematics course of the University of Cambridge 2023 ii Paper 1 5J Solution Created 2026-09-23 Updated 2026-09-25
For , the last flip must be the th head. Among the preceding flips, exactly are tails and are heads. There are choices for their positions, and every resulting sequence has probability . The negative binomial stopping argument therefore givesso has the failures-before-the-th-success negative binomial distribution.
To put the mass function into exponential family form, setSince ,whereThus the natural parameter of an exponential family is , and the Fisher-Neyman factorization theorem shows that is a sufficient statistic. This is the negative binomial exponential family.