As it is a discrete probability function, the Skellam probability mass function is normalized: \sum_{k=-\infty}^\infty p(k;\mu_1,\mu_2) = 1. We know that the
probability generating function (pgf) for a
Poisson distribution is: G\left(t;\mu\right)= e^{\mu(t-1)}. It follows that the pgf, G(t;\mu_1,\mu_2), for a Skellam probability mass function will be: \begin{align} G(t;\mu_1,\mu_2) & = \sum_{k=-\infty}^\infty p(k;\mu_1,\mu_2)t^k \\[4pt] & = G\left(t;\mu_1\right)G\left(1/t;\mu_2\right) \\[4pt] & = e^{-(\mu_1+\mu_2)+\mu_1 t+\mu_2/t}. \end{align} Notice that the form of the
probability-generating function implies that the distribution of the sums or the differences of any number of independent Skellam-distributed variables are again Skellam-distributed. It is sometimes claimed that any linear combination of two Skellam distributed variables are again Skellam-distributed, but this is clearly not true since any multiplier other than \pm 1 would change the
support of the distribution and alter the pattern of
moments in a way that no Skellam distribution can satisfy. The
moment-generating function is given by: M\left(t;\mu_1,\mu_2\right) = G(e^t;\mu_1,\mu_2) = \sum_{k=0}^\infty { t^k \over k!}\,m_k which yields the raw moments
mk . Define: \Delta\ \stackrel{\mathrm{def}}{=}\ \mu_1-\mu_2 \mu\ \stackrel{\mathrm{def}}{=}\ \tfrac{1}{2}(\mu_1+\mu_2). Then the raw moments
mk are \begin{align} m_1 &= \Delta \\ m_2 &= 2\mu + \Delta^2 \\ m_3 &= \Delta \left(1 + 6\mu + \Delta^2\right) \end{align} The
central moments M k are \begin{align} M_2 &= 2\mu, \\ M_3 &= \Delta, \\ M_4 &= 2\mu + 12\mu^2.\, \end{align} The
mean,
variance,
skewness, and
kurtosis excess are respectively: \begin{align} \operatorname E(n) & = \Delta, \\[4pt] \sigma^2 & = 2\mu, \\[4pt] \gamma_1 & = \Delta/(2\mu)^{3/2}, \\[4pt] \gamma_2 & = 1/2. \end{align} The
cumulant-generating function is given by: K(t;\mu_1,\mu_2)\ \stackrel{\mathrm{def}}{=}\ \ln(M(t;\mu_1,\mu_2)) = \sum_{k=0}^\infty \frac{ t^k }{ k!}\,\kappa_k which yields the
cumulants: \begin{align} \kappa_{2k} &= 2\mu, \\ \kappa_{2k+1} &= \Delta . \end{align} For the special case when
μ1 =
μ2, an
asymptotic expansion of the
modified Bessel function of the first kind yields for large
μ: p(k;\mu,\mu)\sim \frac{1}{\sqrt{4\pi\mu}} \left[1 + \sum_{n=1}^\infty \left(-1\right)^n \frac{ \left\{4k^2-1^2\right\} \left\{4k^2-3^2\right\} \cdots \left\{4k^2-(2n-1)^2\right\} }{ n!\,2^{3n}\,(2\mu)^n }\right]. (Abramowitz & Stegun 1972, p. 377). Also, for this special case, when
k is also large, and of
order of the square root of 2
μ, the distribution tends to a
normal distribution: p(k;\mu,\mu) \sim \frac{e^{-k^2/4\mu}}{\sqrt{4\pi\mu}}. These special results can easily be extended to the more general case of different means.
Bounds on weight above zero If {{nowrap|X \sim \operatorname{Skellam} (\mu_1, \mu_2) ,}} with then \frac{\exp\left[-\left(\sqrt{\mu_1} -\sqrt{\mu_2}\right)^2 \right]}{\left(\mu_1 + \mu_2\right)^2} - \frac{e^{-(\mu_1 + \mu_2)}}{2\sqrt{\mu_1 \mu_2}} - \frac{e^{-(\mu_1 + \mu_2)}}{4\mu_1 \mu_2} \leq \Pr\{X \geq 0\} \leq \exp \left[- \left(\sqrt{\mu_1} -\sqrt{\mu_2}\right)^2\right] Details can be found in == See also ==