where is the complementary error function, and is the Laplace function (CDF of the standard normal distribution). The shift parameter has the effect of shifting the curve to the right by an amount and changing the support to the interval [, ). Like all stable distributions, the Lévy distribution has a standard form Template:Nobr which has the following property:
however, this diverges for and is therefore not defined on an interval around zero, so the moment-generating function is actually undefined.
Like all stable distributions except the normal distribution, the wing of the probability density function exhibits heavy tail behavior falling off according to a power law:
as
which shows that the Lévy distribution is not just heavy-tailed but also fat-tailed. This is illustrated in the diagram below, in which the probability density functions for various values of c and are plotted on a log–log plot:
Random samples from the Lévy distribution can be generated using inverse transform sampling. Given a random variate U drawn from the uniform distribution on the unit interval (0, 1], the variate X given by[1]
is Lévy-distributed with location and scale . Here is the cumulative distribution function of the standard normal distribution.
The time of hitting a single point, at distance from the starting point, by the Brownian motion has the Lévy distribution with . (For a Brownian motion with drift, this time may follow an inverse Gaussian distribution, which has the Lévy distribution as a limit.)
The length of the path followed by a photon in a turbid medium follows the Lévy distribution.[2]
Script error: No such module "citation/CS1". - John P. Nolan's introduction to stable distributions, some papers on stable laws, and a free program to compute stable densities, cumulative distribution functions, quantiles, estimate parameters, etc. See especially An introduction to stable distributions, Chapter 1