Natural exponential family
In probability and statistics, a natural exponential family (NEF) is a class of probability distributions that is a special case of an exponential family (EF). Every distribution possessing a moment-generating function is a member of a natural exponential family, and the use of such distributions simplifies the theory and computation of generalized linear models.
The natural exponential family (NEF) is a subset of the exponential family. NEF is an exponential family in which the natural parameter η and the natural statistic T(x) are both the identity. A distribution in the exponential family with parameter θ can be written with probability density function (PDF)
where and are known functions. A distribution in the natural exponential family with parameter θ can thus be written with PDF
[Note that slightly different notation is used by the originator of the NEF, Carl Morris.1 Morris uses ω instead of η and ψ instead of A.]
Suppose that , then a natural exponential family of order p has density or mass function of the form:
where in this case the parameter
A member of a natural exponential family has moment generating function (MGF) of the form
The cumulant generating function is by definition the logarithm of the MGF, so it is
The five most important univariate cases are:
- normal distribution with known variance
- Poisson distribution
- gamma distribution with known shape parameter α (or k depending on notation set used)
- binomial distribution with known number of trials, n
- negative binomial distribution with known
These five examples – Poisson, binomial, negative binomial, normal, and gamma – are a special subset of NEF, called NEF with quadratic variance function (NEF-QVF) because the variance can be written as a quadratic function of the mean. NEF-QVF are discussed below.
Distributions such as the exponential, chi-squared, Rayleigh, Weibull, Bernoulli, and geometric distributions are special cases of the above five distributions. Many common distributions are either NEF or can be related to the NEF. For example: the chi-squared distribution is a special case of the gamma distribution. The Bernoulli distribution is a binomial distribution with n = 1 trial. The exponential distribution is a gamma distribution with shape parameter α = 1 (or k = 1 ). The Rayleigh and Weibull distributions can each be written in terms of an exponential distribution.
The parameterization of most of the above distributions has been written differently than the parameterization commonly used in textbooks and the above linked pages. For example, the above parameterization differs from the parameterization in the linked article in the Poisson case. The two parameterizations are related by , where λ is the mean parameter, and so that the density may be written as
for , so
- , and
This alternative parameterization can greatly simplify calculations in mathematical statistics. For example, in Bayesian inference, a posterior probability distribution is calculated as the product of two distributions. Normally this calculation requires writing out the probability distribution functions (PDF) and integrating; with the above parameterization, however, that calculation can be avoided. Instead, relationships between distributions can be abstracted due to the properties of the NEF described below.
An example of the multivariate case is the multinomial distribution with known number of trials.
The properties of the natural exponential family can be used to simplify calculations involving these distributions.
1. The cumulants of an NEF can be calculated as derivatives of the NEF's cumulant generating function. The nth cumulant is the nth derivative with respect to θ of the cumulant generating function.citation needed
The cumulant generating function is
The first cumulant is
The mean is the first moment and always equal to the first cumulant, so
The variance is always the second moment, and it is always related to the first and second cumulants by
The nth cumulant is
2. Natural exponential families (NEF) are closed under convolution.citation needed
Given independent identically distributed (iid) with distribution from an NEF, then is an NEF, although not necessarily the original NEF. This follows from the properties of the cumulant generating function.
3. The variance function for random variables with an NEF distribution can be written in terms of the mean.citation needed
4. The first two moments of a NEF distribution uniquely specify the distribution within that family of distributions.citation needed
In the multivariate case, the mean vector and covariance matrix arecitation needed
A special case of the natural exponential families are those with quadratic variance functions. Six NEFs have quadratic variance functions (QVF) in which the variance of the distribution can be written as a quadratic function of the mean. These are called NEF-QVF. The properties of these distributions were first described by Carl Morris.2
The six NEF-QVF are written here in increasing complexity of the relationship between variance and mean.
1. The normal distribution with fixed variance is NEF-QVF because the variance is constant. The variance can be written , so variance is a degree 0 function of the mean.
2. The Poisson distribution is NEF-QVF because all Poisson distributions have variance equal to the mean , so variance is a linear function of the mean.
3. The Gamma distribution is NEF-QVF because the mean of the Gamma distribution is and the variance of the Gamma distribution is , so the variance is a quadratic function of the mean.
4. The binomial distribution is NEF-QVF because the mean is and the variance is which can be written in terms of the mean as
5. The negative binomial distribution is NEF-QVF because the mean is and the variance is
The properties of NEF-QVF can simplify calculations that use these distributions.
1. Natural exponential families with quadratic variance functions (NEF-QVF) are closed under convolutions of a linear transformation.citation needed That is, a convolution of a linear transformation of an NEF-QVF is also an NEF-QVF, although not necessarily the original one.
Given independent identically distributed (iid) with distribution from a NEF-QVF. A convolution of a linear transformation of an NEF-QVF is also an NEF-QVF.
Let be the convolution of a linear transformation of X. The mean of Y is . The variance of Y can be written in terms of the variance function of the original NEF-QVF. If the original NEF-QVF had variance function
then the new NEF-QVF has variance function
2. Let and be independent NEF with the same parameter θ and let . Then the conditional distribution of given Y has quadratic variance in Y if and only if and are NEF-QVF. Examples of conditional distributions are the normal, binomial, beta, hypergeometric and geometric distributions, which are not all NEF-QVF.1
3. NEF-QVF have conjugate prior distributions on μ in the Pearson system of distributions (also called the Pearson distribution although the Pearson system of distributions is actually a family of distributions rather than a single distribution.) Examples of conjugate prior distributions of NEF-QVF distributions are the normal, gamma, reciprocal gamma, beta, F-, and t- distributions. Again, these conjugate priors are not all NEF-QVF.1
4. If has an NEF-QVF distribution and μ has a conjugate prior distribution then the marginal distributions are well-known distributions.1
These properties together with the above notation can simplify calculations in mathematical statistics that would normally be done using complicated calculations and calculus.
||This article relies largely or entirely upon a single source. (June 2012)|
||This article needs additional citations for verification. (June 2012)|
- Morris C. (2006) "Natural exponential families", Encyclopedia of Statistical Sciences.
- Morris C. (1982) "Natural exponential families with quadratic variance functions". Ann. Statist., 10(1), 65–80.
- Morris C. (1982) Natural exponential families with quadratic variance functions: statistical theory. Dept of mathematics, Institute of Statistics, University of Texas, Austin.