In probability theory, fractional Brownian motion, also called a fractal Brownian motion, is a generalization of Brownian motion. Unlike classical Brownian motion, the increments of fBm need not be independent. fBm is a continuous-timeGaussian processBH on , that starts at zero, has expectation zero for all t in , and has the following covariance function: where H is a real number in, called the Hurst index or Hurst parameter associated with the fractional Brownian motion. The Hurst exponent describes the raggedness of the resultant motion, with a higher value leading to a smoother motion. It was introduced by. The value of H determines what kind of process the fBm is:
if H = 1/2 then the process is in fact a Brownian motion or Wiener process;
if H < 1/2 then the increments of the process are negatively correlated.
The increment process, X = BH − BH, is known as fractional Gaussian noise. There is also a generalization of fractional Brownian motion: n-th order fractional Brownian motion, abbreviated as n-fBm. n-fBm is a Gaussian, self-similar, non-stationary process whose increments of order n are stationary. For n = 1, n-fBm is classical fBm. Like the Brownian motion that it generalizes, fractional Brownian motion is named after 19th century biologist Robert Brown; fractional Gaussian noise is named after mathematician Carl Friedrich Gauss.
Background and definition
Prior to the introduction of the fractional Brownian motion, used the Riemann-Liouville fractional integral to define the process where integration is with respect to the white noise measuredB. This integral turns out to be ill-suited to applications of fractional Brownian motion because of its over-emphasis of the origin. The idea instead is to use a different fractional integral of white noise to define the process: the Weyl integral for t > 0. The main difference between fractional Brownian motion and regular Brownian motion is that while the increments in Brownian Motion are independent, increments for fractional Brownian motion are not. If H > 1/2, then there is positive autocorrelation: if there is an increasing pattern in the previous steps, then it is likely that the current step will be increasing as well. If H < 1/2, the autocorrelation is negative.
Properties
Self-similarity
The process is self-similar, since in terms of probability distributions: This property is due to the fact that the covariance function is homogeneous of order 2H and can be considered as a fractal property. FBm can also be defined as the unique mean-zero Gaussian process, null at the origin, with stationary and self-similar increments.
As for regular Brownian motion, one can define stochastic integrals with respect to fractional Brownian motion, usually called "fractional stochastic integrals". In general though, unlike integrals with respect to regular Brownian motion, fractional stochastic integrals are not semimartingales.
Frequency-domain interpretation
Just as Brownian motion can be viewed as white noise filtered by , fractional Brownian motion is white noise filtered by .
Sample paths
Practical computer realisations of an , although they are only a finite approximation. The sample paths chosen can be thought of as showing discrete sampled points on an fBm process. Three realizations are shown below, each with 1000 points of an fBm with Hurst parameter 0.75. Realizations of three different types of fBm are shown below, each showing 1000 points, the first with Hurst parameter 0.15, the second with Hurst parameter 0.55, and the third with Hurst parameter 0.95. The higher the Hurst parameter is, the smoother the curve will be.
Method 1 of simulation
One can simulate sample-paths of an fBm using methods for generating stationary Gaussian processes with known covariance function. The simplest method relies on the Cholesky decomposition method of the covariance matrix, which on a grid of size has complexity of order. A more complex, but computationally faster method is the circulant embedding method of. Suppose we want to simulate the values of the fBM at times using the Cholesky decomposition method.