| Parameters μ              {\displaystyle \mu }   location (real)                    α              {\displaystyle \alpha }   tail heaviness (real)                    β              {\displaystyle \beta }   asymmetry parameter (real)                    δ              {\displaystyle \delta }   scale parameter (real)                    γ        =                                            α                              2                                      −                          β                              2                                                          {\displaystyle \gamma ={\sqrt {\alpha ^{2}-\beta ^{2}}}} Support x        ∈        (        −        ∞        ;        +        ∞        )                      {\displaystyle x\in (-\infty ;+\infty )\!} PDF α              δ                              K                                  1                                                            (                α                                                                            δ                                              2                                                              +                    (                    x                    −                    μ                                          )                                              2                                                                                            )                                                    π                                                                    δ                                          2                                                        +                  (                  x                  −                  μ                                      )                                          2                                                                                                                            e                      δ            γ            +            β            (            x            −            μ            )                                {\displaystyle {\frac {\alpha \delta K_{1}\left(\alpha {\sqrt {\delta ^{2}+(x-\mu )^{2}}}\right)}{\pi {\sqrt {\delta ^{2}+(x-\mu )^{2}}}}}\;e^{\delta \gamma +\beta (x-\mu )}}                                K                      j                                {\displaystyle K_{j}}   denotes a modified Bessel function of the third kind Mean μ        +        δ        β                  /                γ              {\displaystyle \mu +\delta \beta /\gamma } Variance δ                  α                      2                                    /                          γ                      3                                {\displaystyle \delta \alpha ^{2}/\gamma ^{3}} Skewness 3        β                  /                (        α                              δ            γ                          )              {\displaystyle 3\beta /(\alpha {\sqrt {\delta \gamma }})} | ||
The normal-inverse Gaussian distribution (NIG) is a continuous probability distribution that is defined as the normal variance-mean mixture where the mixing density is the inverse Gaussian distribution. The NIG distribution was noted by Blaesild in 1977 as a subclass of the generalised hyperbolic distribution discovered by Ole Barndorff-Nielsen, in the next year Barndorff-Nielsen published the NIG in another paper. It was introduced in the mathematical finance literature in 1997.
Contents
The parameters of the normal-inverse Gaussian distribution are often used to construct a heaviness and skewness plot called the NIG-triangle.
Moments
The fact that there is a simple expression for the moment generating function implies that simple expressions for all moments are available.
Linear transformation
This class is closed under affine transformations, since it is a particular case of the Generalized hyperbolic distribution, which has the same property.
Summation
This class is infinitely divisible, since it is a particular case of the Generalized hyperbolic distribution, which has the same property.
Convolution
The class of normal-inverse Gaussian distributions is closed under convolution in the following sense: if                     
Related Distributions
The class of NIG distributions is a flexible system of distributions that includes fat-tailed and skewed distributions, and the normal distribution,                     
Stochastic Process
The normal-inverse Gaussian distribution can also be seen as the marginal distribution of the normal-inverse Gaussian process which provides an alternative way of explicitly constructing it. Starting with a drifting Brownian motion (Wiener process),                     
