B. K O P O C I ´ N S K I (Wroc law)
MULTIVARIATE NEGATIVE BINOMIAL
DISTRIBUTIONS GENERATED BY MULTIVARIATE EXPONENTIAL DISTRIBUTIONS
Abstract. We define a multivariate negative binomial distribution (MVNB) as a bivariate Poisson distribution function mixed with a mul- tivariate exponential (MVE) distribution. We focus on the class of MVNB distributions generated by Marshall–Olkin MVE distributions. For simplic- ity of notation we analyze in detail the class of bivariate (BVNB) distribu- tions. In applications the standard data from [2] and [7] and data concerning parasites of birds from [4] are used.
1. Introduction. It is known that a univariate geometrical probability distribution function is a mixed Poisson distribution with exponentially dis- tributed parameter. A univariate negative binomial distribution is a mixed Poisson distribution where the mixing parameter has a gamma distribution.
Also it is easy to see, considering convolution and mixture, that mutually corresponding are: the class of negative binomial distributions and the class of gamma distributions. These univariate properties suggest the definition of a multivariate negative binomial (MVNB) distribution on the basis of multivariate exponential (MVE) distributions and convolution. There exist a few variants of MVE distributions with exponential marginals; we focus on the class of Marshall–Olkin MVE distributions. For simplicity of notation we consider in detail bivariate (BVNB) distributions defined by the BVE class.
We present three applications of BVNB distributions using the standard data from [2] and [7] concerning accidents, and the data concerning the number of parasites of the pheasant [4]. A new variant of MVNB distri-
1991 Mathematics Subject Classification: Primary 62H05; Secondary 62F10.
Key words and phrases: bivariate geometrical distribution, multivariate exponential distribution, multivariate negative binomial distribution.
[463]
butions for random variables characterized by a small correlation may be useful.
In [7] the existence of a negative correlated MVNB distribution is sug- gested. In an example a negative correlated BVNB distribution is shown.
We also present an example of a bivariate distribution with negative bino- mial marginals which do not belong to any class of BVNB distributions.
2. The negative binomial distribution. Let us recall the elementary notations and definitions concerning univariate negative binomial distribu- tions, suitable for the construction of a multivariate analogue. A random variable X is geometrically distributed with parameter p if P (X = k) = qp k , k ≥ 0, 0 < p < 1, q = 1 − p. Its probability generating function (pgf) is φ p (u) = q(1 − pu) −1 , and also we have E(X) = pq −1 , Var(X) = pq −2 . The random variable X is negative binomial with parameters p and r if X = E d Λ (Π(Λ)), where Π(Λ) under the condition Λ = λ is a Poisson ran- dom variable with parameter λ, and Λ has a gamma distribution with shape parameter r and scale parameter p. Its pgf is φ p,r (u) = φ r p (u). The param- eter r is also called aggregation. This random variable has
(1) E(X) = rpq −1 , Var(X) = rpq −2 .
The random variables (Λ 1 , Λ 2 ) have a Marshall–Olkin BVE distribution [6] if there exist random variables U , V , W , mutually independent and exponentially distributed with parameters α ≥ 0, β ≥ 0, γ ≥ 0, respectively, α + β + γ > 0, such that Λ 1 = min(U, W ), Λ 2 = min(V, W ). The
(2) P (Λ 1 > x, Λ 2 > y) = exp(−αx − βy − γ max(x, y)), x ≥ 0, y ≥ 0.
We say that (X 1 , X 2 ) are generated by (Λ 1 , Λ 2 ) if
(3) (X 1 , X 2 ) = E d (Λ 1 ,Λ 2 ) (Π 1 (Λ 1 ), Π 2 (Λ 2 )) df = T (Λ 1 , Λ 2 ),
where Π 1 (Λ 1 ), Π 2 (Λ 2 ) under the condition Λ 1 = λ 1 , Λ 2 = λ 2 are indepen- dent Poisson random variables with parameters λ 1 , λ 2 , respectively. The relation (3) defines a transformation of the distributions of random variables which we also call a transformation of random variables.
Definition 1. The random variables (X 1 , X 2 ) have a bivariate geomet- rical distribution if they are generated by (Λ 1 , Λ 2 ) which have a BVE dis- tribution:
(4) P (X 1 = i, X 2 = j) = E(p(i, Λ 1 )p(j, Λ 2 )), i, j ≥ 0, where p(i, λ) = (λ i /i!)e −λ , i ≥ 0, λ > 0.
Proposition 1. If (Λ 1 , Λ 2 ) has a BVE distribution,
ψ(s, t) = E(exp(−sΛ 1 − tΛ 2 ))
is the Laplace–Stieltjes transform and (X 1 , X 2 ) is generated by (Λ 1 , Λ 2 ), then its pgf is
(5) φ(u, v) = E(u X 1 v X 2 ) = ψ(1 − u, 1 − v).
Moreover ,
E(X i ) = E(Λ i ), Var(X i ) = Var(Λ i ) + E(Λ i ), i = 1, 2, Cov(X 1 , X 2 ) = Cov(Λ 1 , Λ 2 ).
The proof is omitted.
Definition 2. The random variable (X 1 , X 2 ) has a BVNB distribution with aggregation r if its pgf is
(6) φ r (u, v) = E(u X 1 v X 2 ) = φ r (u, v),
where φ(u, v) is the pgf of a bivariate geometrical distribution.
The pgf of a bivariate geometrical distribution function may be presented in terms of the pgf of the univariate geometrical distribution.
Proposition 2. If (Λ 1 , Λ 2 ) is the BVE distribution (2), then the distri- bution function (5) is geometrical and it has the pgf
φ(u, v) = φ α (u)φ β (v) + γ
α + γ φ α (u)φ α+γ (u)φ β (v) (7)
+ γ
β + γ φ α (u)φ β (v)φ β+γ (v)
+ γ
α + β + γ φ α (u)φ β (v)φ 1+α+β+γ (u + v), where φ = 1 − φ.
P r o o f. The Laplace–Stieltjes transform of the BVE distribution (2) (see [6]) is
ψ(s, t) = E(exp(−sΛ 1 − tΛ 2 ))
= (α + β + γ + s + t)(α + γ)(β + γ) + stγ (α + β + γ + s + t)(α + γ + s)(β + γ + t) . Thus, by (5), the result can be restated as
φ(u, v) = 1
(1 − u + α)(1 − v + β)
αβ + γβ 1 − u 1 − u + α + γ + γα 1 − v
1 − v + β + γ + γ (1 − u)(1 − v) 2 − u − v + α + β + γ
.
Proposition 3. If (X 1 , X 2 ) has a BVNB distribution generated by
(Λ 1 , Λ 2 ) with BVE distribution with aggregation r, then
(8)
E(X i ) = rE(Λ i ), Var(X i ) = r Var(Λ i ) + rE(Λ i ), i = 1, 2, Cov(X 1 , X 2 ) = r Cov(Λ 1 , Λ 2 ),
P (X 1 = 0, X 2 = 0) =
(2 + α + β + γ)(α + γ)(β + γ) + γ (2 + α + β + γ)(1 + α + γ)(1 + β + γ)
r
. It is well known [6] that (Λ 1 , Λ 2 ) distributed as (2) has
(9)
E(Λ 1 ) = 1
α + γ , E(Λ 2 ) = 1 β + γ , Cov(Λ 1 , Λ 2 ) = γ
(α + γ)(β + γ)(α + β + γ) .
Example 1. Let (Λ 1 , Λ 2 ) = (α 1 U, α 2 U ), where α 1 > 0, α 2 > 0, and U is exponentially distributed with parameter γ > 0. Then the density function of (U, U ) is singular, f (u, u) = γe −γu , u > 0. From (4) for i ≥ 0, j ≥ 0 we have
P (X 1 = i, X 2 = j) =
∞
\