Home > Completeness (statistics)

(X₁, ..., X_n) of scalar-valued random variables), has a probability distribution belonging to a known family of probability distributions, parametrized by θ, which may be either vector- or scalar-valued. A function g(X) is an unbiased estimator of zero if the expectation E(g(X)) remains zero regardless of the value of the parameter θ. Then X is a complete statistic precisely if it admits no such unbiased estimator of zero.

For example, suppose X₁, X₂ are independent, identically distributed random variables,

expecation θ and variance 1. Then X₁ — X₂ is an unbiased estimator of zero. Therefore the pair (X₁, X₂) is not a complete statistic. On the other hand, the sum X₁ + X₂ can be shown to be a complete statistic. That means that there is no non-zero function g such that

remains zero regardless of changes in the value of θ. That fact may be seen as follows. The probability distribution of X₁ + X₂ is normal with expectation 2θ and variance 2. Its probability density function is therefore

The expectation above would therefore be a constant times

A bit of algebra reduces this to

As a function of θ this is a two-sided Laplace transform of h(x), and cannot be identically zero unless h(x) zero almost everywhere.

One reason for the importance of the concept is the Lehmann-Scheffé theorem, which states that a statistic that is complete, sufficient, and unbiased is the best unbiased estimator, i.e., the one that has a smaller mean squared error than any other unbiased estimator, or, more generally, a smaller expected loss, for any convex loss function.